How Massive Single Stars End their Life

Abstract

How massive stars die -- what sort of explosion and remnant each produces -- depends chiefly on the masses of their helium cores and hydrogen envelopes at death. For single stars, stellar winds are the only means of mass loss, and these are chiefly a function of the metallicity of the star. We discuss how metallicity, and a simplified prescription for its effect on mass loss, affects the evolution and final fate of massive stars. We map, as a function of mass and metallicity, where black holes and neutron stars are likely to form and where different types of supernovae are produced. Integrating over an initial mass function, we derive the relative populations as a function of metallicity. Provided single stars rotate rapidly enough at death, we speculate upon stellar populations that might produce gamma-ray bursts and jet-driven supernovae.

24 pages, 9 figues, submitted to ApJ

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• The Formation of the First Massive Black Holes
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• Genesis and evolution of dust in galaxies in the early Universe I. Modeling dust evolution in starburst galaxies
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• SN2011hs: a Fast and Faint Type IIb Supernova from a Supergiant Progenitor
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• Photometric and Spectroscopic Evolution of the Type IIP SN 2007it to Day 944
• Jumping the gap: searching for LIGO's biggest black holes
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• Star Formation in the First Galaxies - II: Clustered Star Formation and the Influence of Metal Line Cooling
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• The Population III origin of GW190521
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• The diffuse $\gamma$-ray background is dominated by star-forming galaxies
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• Constraining Globular Cluster Formation Through Studies of Young Massive Clusters - IV. Testing the Fast Rotating Massive Star Scenario
• The Birth of an Ultra-Luminous X-ray Source in M83
• Gravitational wave sources in the era of multi-frequency gravitational wave astronomy
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• Chandra Survey of Nearby Galaxies: The Catalog
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• Supernova Nebular Spectroscopy Suggests a Hybrid Envelope-Stripping Mechanism for Massive Stars
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• SN 2011fu: A type IIb Supernova with a luminous double-peaked light curve
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• Constraints for the Progenitor Masses of 17 Historic Core-Collapse Supernovae
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• Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-Envelope Core-Collapse Supernovae
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• Outflows of stars due to quasar feedback
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• Gravitational wave of intermediate-mass black holes in Population III star clusters
• Chandra and XMM-Newton imaging and spectroscopic study of the supernova remnant Kes 73 hosting the magnetar 1E 1841-045
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• Nearby supernova host galaxies from the CALIFA Survey: II. SN environmental metallicity
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• GW150914-like Black Holes as Galactic High-Energy Sources
• Chandra and XMM-Newton studies of the supernova remnant G292.2-0.5 associated with the pulsar J1119-6127
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• Neutrino-Driven Explosions in GRBs and Hypernovae
• The Dusty and Extremely Red Progenitor of the Type II Supernova 2023ixf in Messier 101
• Trojan Stars in the Galactic Center
• Constraints on Type IIn Supernova Progenitor Outbursts from the Lick Observatory Supernova Search
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• Supernovae and their host galaxies - II. The relative frequencies of supernovae types in spirals
• Testing the predicted mass-loss bi-stability jump at radio wavelengths
• Progenitor Mass Distribution of Core-Collapse Supernova Remnants in Our Galaxy and Magellanic Clouds based on Elemental Abundances
• ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• The Lack of Gamma-Ray Bursts from Population III Binaries
• The Properties of the Progenitor Supernova, Pulsar Wind, and Neutron Star inside PWN G54.1+0.3
• A new constraint for gamma-ray burst progenitor mass
• The Radio to Infrared Emission of Very High Redshift Gamma-Ray Bursts: Probing Early Star Formation through Molecular and Atomic Absorption Lines
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• The Redshift Distribution of Distant Supernovae and its Use in Probing Reionization
• A Multiple Ejecta-Circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc
• XMM-Newton observation of PSR B2224+65 and its jet
• Supernova rates from the SUDARE VST-Omegacam search II. Rates in a galaxy sample
• The effect of baryonic streaming motions on the formation of the first supermassive black holes
• Using failed supernovae to constrain the Galactic r-process element production
• SN 2007uy - metamorphosis of an aspheric Type Ib explosion
• Angular momentum transfer in primordial discs and the rotation of the first stars
• Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
• Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud
• Growing Massive Black Holes in a Local Group Environment: the Central Supermassive, Slowly Sinking, and Ejected Populations
• Evidence for a Black Hole Remnant in the Type IIL Supernova 1979C
• The First Stars: formation under X-ray feedback
• Neutrino spin oscillations in matter under the influence of gravitational and electromagnetic fields
• The birthplace and age of the isolated neutron star RX J1856.5-3754
• Radiation Hydrodynamical Simulations of the Birth of Intermediate-Mass Black Holes in the First Galaxies
• On the Contribution of Gamma Ray Bursts to the Galactic Inventory of Some Intermediate Mass Nuclei
• A Central Excess of Stripped-Envelope Supernovae within Disturbed Galaxies
• Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au
• Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C
• Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
• Influence of Population III stars on cosmic chemical evolution
• Impact of metallicity on the evolution of young star clusters
• Why are pulsar planets rare?
• Feedback from the IR Background in the Early Universe
• Cosmography with next-generation gravitational wave detectors
• Dark Matter Accretion into Supermassive Black Holes
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• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
• SNe 2013K and 2013am: observed and physical properties of two slow, normal Type IIP events
• Neutrinos from failed supernovae at future water and liquid argon detectors
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• Nucleosynthetic Constraints on the Mass of the Heaviest Supernovae
• Impact of new data for neutron-rich heavy nuclei on theoretical models for $r$-process nucleosynthesis
• The ultraluminous X-ray source population of NGC 4485/4490
• Formation of High-redshift (z>6) Quasars Driven by Nuclear Starbursts
• A Study of Primordial Very Massive Star Evolution
• The Impact of Black Hole Formation on Population Averaged Supernova Yields
• Multiband counterparts of two eclipsing ultraluminous X-ray sources in M 51
• Chemical evolution of elliptical galaxies with a variable IMF -- A publicly available code
• The diversity of supernovae and impostors shortly after explosion
• Cosmic backgrounds due to the formation of the first generation of supermassive black holes
• Highlights and Discoveries from the Chandra X-ray Observatory
• Review of scientific topics for Millimetron space observatory
• Long-Duration Gamma-Ray Burst Host Galaxies in Emission and Absorption
• Evolution and CNO yields of Z=10^-5 stars and possible effects on CEMP production
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• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• The disappearance of the progenitor of SN 2012aw in late-time imaging
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• First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics
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• On the Existence of Pulsars in the Vicinity of the Massive Black Hole in the Galactic Center
• High Energy neutrino signals from the Epoch of Reionization
• A self-consistent semi-analytic model for Population III star formation in minihalos
• Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33
• The effects of stellar winds of fast-rotating massive stars in the earliest phases of the chemical enrichment of the Galaxy
• The r-Process in Metal Poor Stars and Black Hole Formation
• Binary companions of nearby supernova remnants found with Gaia
• The dusty aftermath of SN Hunt248: merger-burst remnant?
• Stellar winds and metal enrichment from fast-rotating Population III stars
• The WMAP haze from the Galactic Center region due to massive star explosions and a reduced cosmic ray scale height
• Evidence for magnetar formation in broad-lined type Ic supernovae 1998bw and 2002ap
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Suppression of accretion onto low-mass Population III stars
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• Search for Gamma-rays from Dark Matter annihilations around Intermediate Mass Black Holes with the H.E.S.S. experiment
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
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• An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
• No surviving stellar companion for Cassiopeia A
• Type Ia Supernovae: Colors, Rates, and Progenitors
• Exploring the effects of pressure on the radial accretion of dark matter by a Schwarzschild supermassive black hole
• Fisher vs. Bayes : A comparison of parameter estimation techniques for massive black hole binaries to high redshifts with eLISA
• Final compact remnants in core-collapse supernovae from 20 to 40 $M_{\odot }$: the lower mass gap
• The observed neutron star mass distribution as a probe of the supernova explosion mechanism
• A VLA Study of High-redshift GRBs I - Multi-wavelength Observations and Modeling of GRB 140311A
• Open-cluster density profiles derived using a kernel estimator
• Probing the Shock Breakout Signal of SN 2024ggi from the Transformation of Early Flash Spectroscopy
• A search for radio pulsars and fast transients in M31 using the WSRT
• Photometric and polarimetric observations of fast declining Type II supernovae 2013hj and 2014G
• Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
• Type IIP supernova 2008in: the explosion of a normal red supergiant
• A UV census of the environments of stripped-envelope supernovae
• Emission-line Wings Driven by Lyman Continuum in the Green Pea Analog Mrk 71
• X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Designing a cross-correlation search for continuous-wave gravitational radiation from a neutron star in the supernova remnant SNR 1987A
• An Unusual Mid-Infrared Flare in a Type 2 AGN: An Obscured Turning-on AGN or Tidal Disruption Event?
• OB Associations, Wolf-Rayet Stars, and the Origin of Galactic Cosmic Rays
• Rapid neutron star cooling triggered by dark matter
• Type IIP Supernova 2009kf: Explosion Driven by Black Hole Accretion?
• CXOM31 J004253.1+411422: The first ultra-luminous X-ray transient in M 31
• Early chemical enrichment of the universe and the role of very massive pop III stars
• The impact of realistic red supergiant mass-loss on stellar evolution
• Ejecta and progenitor of the low-luminosity Type IIP supernova 2003Z
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• Growth of stellar mass black holes in dense molecular clouds and GW190521
• Supernovae and Cosmology
• New Test of Supernova Electron Neutrino Emission using Sudbury Neutrino Observatory Sensitivity to the Diffuse Supernova Neutrino Background
• Convectively Driven Three Dimensional Turbulence in Massive Star Envelopes: I. A 1D Implementation of Diffusive Radiative Transport
• Radiative Regulation of Population III Star Formation
• Recycled pulsars with black hole companions: the high mass analogues of PSR B2303+46
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Population III Hypernovae
• The fingerprint of binary intermediate mass black holes in globular clusters: supra-thermal stars and angular momentum alignment
• Supernovae and the Chirality of the Amino Acids
• The Connection Between X-ray Binaries and Star Clusters in NGC 4449
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
• SN 2012ca: a stripped envelope core-collapse SN interacting with dense circumstellar medium
• Supernova explosions of massive stars and cosmic rays
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• Observational evidence for a correlation between peak-luminosities and beaming in GRBs
• Studying Relation Between Star Formation and Molecular Clumps on Subparsec Scales in 30 Doradus
• Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A
• A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Low luminosity Type II supernovae III. SN 2018hwm, a faint event with an unusually long plateau
• Progenitor properties of type II supernovae: fitting to hydrodynamical models using Markov chain Monte Carlo methods
• Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr
• A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars: II. The northern WNE sequence
• The Energy Sources of Superluminous Supernovae
• An Observational Limit on the Earliest GRBs
• The population of merging compact binaries inferred using gravitational waves through GWTC-3
• Searching for a magnetic field in Wolf-Rayet stars using FORS2 spectropolarimetry
• Mass-loss predictions for evolved very metal-poor massive stars
• Multiwavelength analysis of three SNe associated with GRBs observed by GROND
• X-Ray Luminous Binaries, Metallicity, and the Early Universe
• The oldest X-ray supernovae: X-ray emission from 1941C, 1959D, 1968D
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• Average opacity calculation for core-collapse supernovae
• Population III Star Clusters in the Reionized Universe
• Optical and Ultraviolet Observations of the Very Young Type IIP SN 2014cx in NGC 337
• Nuclear processes in Astrophysics: Recent progress
• On the multiplicity of supernovae within host galaxies
• Close Encounters of Wide Binaries Induced by the Galactic Tide: Implications for Stellar Mergers and Gravitational-Wave Sources
• Phase-dependent study of near-infrared disk emission lines in LB-1
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• Cosmic infrared background from Population III stars and its effect on spectra of high-z gamma-ray bursts
• The Role of Primordial Kicks on Black Hole Merger Rates
• The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
• Possibility of QCD critical point sweep during black hole formation
• The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge
• Massive Stars and their Supernovae
• Role of supergiants in the formation of globular clusters
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• Explodability criteria for the neutrino-driven supernova mechanism
• Black hole hyperaccretion inflow-outflow model. II. Long-duration gamma-ray bursts and supernova ${}^{56}\mathrm{Ni}$ bumps
• Binary parameters from astrometric and spectroscopic errors--candidate hierarchical triples and massive dark companions in Gaia DR3
• SN 2017ivv: two years of evolution of a transitional Type II supernova
• Population III X-ray Binaries and their Impact on the Early Universe
• Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
• The statistical investigation of type Ib/c and II supernovae and their host galaxies
• Supernova 2018cuf: A Type IIP supernova with a slow fall from plateau
• Neutrino Signatures from the First Stars
• Mining for Candidates of Galactic Stellar-mass Black Hole Binaries with LAMOST
• On extreme transient events from rotating black holes and their gravitational wave emission
• Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)
• Gravitational Wave Signals from the First Massive Black Hole Seeds
• Supernovae from massive stars
• The first Infrared study of the close environment of a long Gamma-Ray Burst
• X-Ray emission from SN 2004dj: A Tale of Two Shocks
• Gravitational Wave Signal from Assembling the Lightest Supermassive Black Holes
• Gravitational waves from intermediate-mass black holes in young clusters
• A Sub-Solar Metallicity Progenitor for Cassiopeia A, the remnant of a Type IIb Supernova
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• Cosmography with Standard Sirens from the Einstein Telescope
• The Origin of Cosmic Rays: How Their Composition Defines Their Sources and Sites, and the Processes of Their Mixing, Injection and Acceleration
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• The Non-Monotonic Dependence of Supernova and Remnant Formation on Progenitor Rotation
• Quantifying the energy balance between the turbulent ionised gas and young stars
• Modelling the chemical enrichment of Population III supernovae: The origin of the metals in near-pristine gas clouds
• Broad band polarimetric investigation of Type IIP supernova 2013ej
• Numerical and analytical solutions of Neutrino-Dominated Accretion Flows with a Non-Zero Torque Boundary Condition and its applications in Gamma-ray Bursts
• Constraining the mass of the GRB 030329 progenitor
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• The role of stellar expansion on the formation of gravitational wave sources
• A high fraction of close massive binary stars at low metallicity
• Exploring the impact of IMF and binary parameter stochasticity with a binary population synthesis code
• Evidence for multiple origins of fast declining Type II supernovae from spectropolarimetry of SN 2013ej and SN 2017ahn
• Hot Cores : Probes of High-Redshift Galaxies
• ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy
• Observing the First Stars and Black Holes
• Fields from a relativistic magnetic explosion
• Updated Photometry of the Yellow Supergiant Progenitor and Late-time Observations of the Type IIb Supernova 2016gkg
• Properties of High-Redshift GRBs
• Lepton Flavour Asymmetries and the Mass Spectrum of Primordial Black Holes
• Supernovae Powered by Collapsar Accretion in Gamma-Ray Burst Sources
• The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• Cosmic Ray production of Beryllium and Boron at high redshift
• The Formation and Evolution of the First Massive Black Holes
• Effects of QCD phase transition on gravitational radiation from two-dimensional collapse and bounce of massive stars
• Interactions between Ultra-High-Energy Particles and Protogalactic Environments
• SN 2015ba: A type IIP supernova with a long plateau
• The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars
• SN 2018hna: 1987A-like supernova with a signature of shock breakout
• ASASSN-16fp (SN 2016coi): A transitional supernova between Type Ic and broad-lined Ic
• Dust masses of $z>5$ galaxies from SED fitting and ALMA upper limits
• White Dwarf Bounds on CHAMPs
• PS15cey and PS17cke: prospective candidates from the Pan-STARRS Search for Kilonovae
• Mergers of Equal-Mass Binaries with Compact Object Companions from Mass Transfer in Triple Star Systems
• Optical studies of two stripped envelope supernovae SN 2015ap (Type Ib) and SN 2016P (Type Ic)
• How is Binary Radio-Pulsars with Black Holes Population Rich?
• The impact of ionizing radiation on the formation of a supermassive star in the early Universe
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• Dynamics of massive stellar black holes in young star clusters and the displacement of ultra-luminous X-ray sources
• Enhanced star formation in $z\sim 6$ quasar companions
• Supernova progenitor stars in the initial range of 23 to 33 solar masses and their relation with the SNR Cas A
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• Discovery of the Near-IR Afterglow and of the Host of GRB 030528
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• Gamma Ray Burst studies with THESEUS
• A Multi-Wavelength View on the Rapidly-Evolving Supernova 2018ivc: An Analog of SN IIb 1993J but Powered Primarily by Circumstellar Interaction
• SN 2008gz - most likely a normal type IIP event
• Numerical Study on Stellar Core Collapse and Neutrino Emission: Probe into the Spherically Symmetric Black Hole Progenitors with 3 - 30Msun Iron Cores
• UV regulated star formation in high-redshift galaxies
• Observational signature of circumstellar interaction and ${}^{56}$Ni-mixing in the Type II Supernova 2016gfy
• Radio Analysis of SN 2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse
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• X-Shooting ULLYSES: Massive Stars at low metallicity IX: Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
• The Gravitational Wave Signature of Core-Collapse Supernovae
• Searching for Hydrogen in Type Ib Supernovae
• VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), sigma Oph, BM Sco, and HD 206859
• The Cosmic MeV Neutrino Background as a Laboratory for Black Hole Formation
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Powering luminous core collapse supernovae with jets
• X-ray Binaries and Star Clusters in the Antennae: Optical Cluster Counterparts
• Simulations of Accretion Powered Supernovae in the Progenitors of Gamma Ray Bursts
• High Energy Neutrino Emission from the Earliest Gamma-Ray Bursts
• Black Holes in our Galactic Halo: Compatibility with FGST and PAMELA Data and Constraints on the First Stars
• The X-Ray Point-Source Population of NGC 1365: The Puzzle of Two Highly-Variable Ultraluminous X-ray Sources
• Impact of magnetic fields on Population III star formation
• SN 2018ijp: the explosion of a stripped-envelope star within a dense H-rich shell?
• Long Gamma Ray Bursts from binary black holes
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• A search for hyperluminous X-ray sources in the XMM-Newton source catalog
• Dust evolution processes constrained by extinction curves in nearby galaxies
• Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernova
• The Transient High-Energy Sky and Early Universe Surveyor (THESEUS)
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• Constraining Type Iax Supernova Progenitor Systems with Stellar Population Aging
• On the association of ULXs with young superclusters: M82 X-1 and a new candidate in NGC 7479
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• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
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• GRB-SN Association within the Binary-Driven Hypernova Model
• Dynamical Friction in a Gas: The Supersonic Case
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• Resolving the puzzle of type IIP SN 2016X
• SN 2016gsd: An unusually luminous and linear type II supernova with high velocities
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• The Origin of the Young Pulsar PSR J0826+2637 and Its Possible Former Companion HIP 13962
• Gamma-ray Bursts and the Early Star-formation History
• The best place and time to live in the Milky Way
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• Radio Supernovae in the Great Survey Era
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• Is there room for highly magnetized pulsar wind nebulae among those non-detected at TeV?
• Black Holes In Young Stellar Clusters
• Supernova Neutrino-Effects on R-Process Nucleosynthesis in Black Hole Formation
• Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion
• On the operation of the chemothermal instability in primordial star-forming clouds
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• The impact of asymmetric dark matter on the thermal evolution of nucleonic and hyperonic compact stars
• Detection of Gravitational Waves from the Coalescence of Population-III Remnants with Advanced LIGO
• The First Stars: formation under cosmic ray feedback
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• Gravitational Waves from Disks Around Spinning Black Holes: Simulations in Full General Relativity
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• A practical guide to the massive black hole cosmic history
• A cosmic formation site of silicon and sulphur revealed by a new type of supernova explosion
• Light element variations in globular clusters via nucleosynthesis in black hole accretion discs
• Universe opacity and CMB
• Little Red Dots Are Nurseries of Massive Black Holes
• The Impact of Initial-Final Mass Relations on Black Hole Microlensing
• A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A
• Merging binary black holes formed through double-core evolution
• Young rotation-powered pulsars as ultra-luminous X-ray sources
• LMC X-1: A New Spectral Analysis of the O-star in the binary and surrounding nebula
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• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
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• A search for \textit{Fermi} bursts associated to supernovae and their frequency of occurrence
• Dynamically Formed Black Hole Binaries: In-Cluster Versus Ejected Mergers
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• Implications of recoil kicks for black hole mergers from LIGO/Virgo catalogs
• The rapid decay phase of the afterglow as the signature of the Blandford-Znajek mechanism
• Experimental Constraint on Stellar Electron-Capture Rates from the ${}^{88}\text{Sr}(t,{}^3\text{He}+\gamma ){}^{88}\text{Rb}$ reaction at 115 MeV/u
• Remnants of massive metal-poor stars: viable engines for ultra-luminous X-ray sources
• Collective Properties of X-ray Binary Populations of Galaxies. I. Luminosity and Orbital Period Distributions of High-Mass X-ray Binaries
• No WIMP Mini-Spikes in Dwarf Spheroidal Galaxies
• Imprint of Gravitational Lensing by Population III Stars in Gamma Ray Burst Light Curves
• VIRGO sensitivity to binary coalescences and the Population III black hole binaries
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• A 3D short-characteristics method for continuum and line scattering problems in the winds of hot stars
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• The giants that were born swiftly -- Implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
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• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Unveiling the Nature of SN 2011fh: a Young and Massive Star Gives Rise to a Luminous SN 2009ip-like Event
• Influence of macroclumping on type II supernova light curves
• A systematic study of magnetar-powered hydrogen-rich supernovae
• The zenithal 4-m International Liquid Mirror Telescope: a unique facility for supernova studies
• ASASSN-15no: The Supernova that plays hide-and-seek
• Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
• Simultaneous VLBA polarimetric observations of the v=$\{$1,2$\}$ J=1-0 and v=1, J=2-1 SiO maser emission toward VY CMa II: component-level polarization analysis
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• Nucleosynthesis in the outflows associated with accretion disks of Type II collapsars
• Near-Infrared Spectroscopy of Infrared-Excess Stellar Objects in the Young Supernova Remnant G54.1+0.3
• Comprehensive multi-wavelength modelling of the afterglow of GRB050525A
• Supernovae and Gaia
• Pregalactic LiBeB Production by Supernova Cosmic Rays
• The Reionization History and Early Metal Enrichment inferred from the Gamma-Ray Burst Rate
• Formation of Massive Black Holes in Globular Clusters
• Supergiants and their shells in young globular clusters
• A metallicity dependence on the occurrence of core-collapse supernovae
• GRBs and fundamental physics
• DES16C3cje: A low-luminosity, long-lived supernova
• Supernovae Shock Breakout/Emergence Detection Predictions for a Wide-Field X-ray Survey
• Footprints of population III stars in the gravitational-wave background
• Core-collapse supernova subtypes in luminous infrared galaxies
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• The Galactic Spatial Distribution of OB Associations and Their Surrounding Supernova-Generated Superbubble
• The jittering jets explosion mechanism (JJEM) in electron capture supernovae
• SOFIA Observations of SN 2010jl: Another Non-Detection of the 9.7 $\mu$m Silicate Dust Feature
• The effects of Time-Variable Absorption due to Gamma-Ray Bursts In Active Galactic Nuclei Accretion Disks
• Revisiting the progenitor of the low-luminosity type II-plateau supernova, SN 2008bk
• SN 1961V: A Pulsational Pair-Instability Supernova
• A LOFAR search for steep-spectrum pulsars in Supernova Remnants and Pulsar Wind Nebulae
• Star formation history, double degenerates and type Ia supernovae in the thin disc
• The radial distribution of supernovae compared to star formation tracers
• Galactic Constraints on Supernova Progenitor Models
• First Light II: Emission Line Extinction, Population III Stars, and X-ray Binaries
• Detection of LIGO-Virgo binary black holes in the pair-instability mass gap
• Supernovae without host galaxy? - Hypervelocity stars in foreign galaxies
• Neutron stars formation and Core Collapse Supernovae
• Internal heating mechanisms in neutron stars
• Computational Models of Stellar Collapse and Core-Collapse Supernovae
• SiO and H2O Maser Observations of Red Supergiants in Star Clusters Embedded in the Galactic Disk
• The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
• A ULX associated with a cloud collision in M99
• Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies
• Finding $\eta$ Car Analogs in Nearby Galaxies Using Spitzer: II. Identification of An Emerging Class of Extragalactic Self-Obscured Stars
• Constraints on Gamma-ray Burst Inner Engines in a Blandford-Znajek Framework
• Vibrational instability of Population III very massive main-sequence stars due to the $\epsilon$-mechanism
• The superimposed photospheric and stellar wind variability of the O-type supergiant alpha Cam
• The Impact of metallicity evolution of the universe on the maximum mass of LIGO binary black holes
• The first days of type II-P core collapse supernovae in the gamma-ray range
• Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
• The radio pulsar population of the Small Magellanic Cloud
• Evolution of rotating massive stars with new hydrodynamic wind models
• X-ray emission from star cluster winds in starburst galaxies
• Neutrino-dominated accretion flows: second nucleosynthesis factory in core-collapse supernovae and regulation of iron markets in galaxies
• Repeated mergers of black hole binaries: implications for GW190521
• Supernovae without host galaxies? The low surface brightness host of SN 2009Z
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches
• Spitzer observations of the N157B supernova remnant and its surroundings
• Distinguishing the impact and signature of black holes from different origins in early cosmic history
• Evolution of neutron star + He star binaries: an alternative evolutionary channel to intermediate-mass binary pulsars
• Light Curves and Spectra from a Unimodal Core-Collapse SuperNova
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• iPTF14hls in the circumstellar medium interaction model: A promising candidate for a pulsational pair-instability supernova
• Stability and instability of strange dwarfs
• Magnesium-rich Ejecta in the SNR G284.3$-$1.8 Around the High-Mass Gamma-Ray Binary 1FGL J1018.6$-$5856
• Multiwavelength Scrutiny of X-ray Sources in Dwarf Galaxies: ULXs versus AGN
• Growth of Intermediate Massive Black Holes in the Hierarchical Formation of Small Spiral Galaxies in the High-z Universe
• A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
• Triggering the formation of direct collapse black holes by their congeners
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Mechanical feedback from black hole accretion as an energy source of core-collapse supernova explosions
• Accreting Black Holes
• The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051
• A Quark-Nova in the wake of a core-collapse Supernova: a unifying model for long duration Gamma-Ray Bursts and Fast Radio Bursts
• A model for microquasars of Population III
• VLTI-PIONIER imaging of the red supergiant V602 Carinae
• Massive black hole formation in Population III star clusters
• No supernovae detected in two long-duration Gamma-Ray Bursts
• Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo
• Accretion onto Intermediate-mass Seed Black Holes in Primordial Galaxies
• Enhanced Detectability of Pre-reionization 21-cm Structure
• Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity
• The growth of supermassive black holes fed by accretion disks
• SN 2017czd: A Rapidly Evolving Supernova from a Weak Explosion of a Type IIb Supernova Progenitor
• Disentangling the Black Hole Mass Spectrum with Photometric Microlensing Surveys
• Presupernova Structure of Massive Stars
• Comparing Moment-Based and Monte Carlo Methods of Radiation Transport Modeling for Type II-Plateau Supernova Light Curves
• The population synthesis of Wolf-Rayet stars involving binary merger channels
• The origin of the Guitar pulsar
• Signatures of very massive stars: supercollapsars and their cosmological rate
• On the dynamical formation of accreting intermediate mass black holes
• Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
• Premature Black Hole Death of Population III Stars by Dark Matter
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Observing the Galactic Underworld: Predicting photometry and astrometry from compact remnant microlensing events
• Magnetar central engines in gamma-ray busts follow the universal relation of accreting magnetic stars
• Neutrino oscillations in magnetically driven supernova explosions
• Wolf-Rayet stars, black holes and the first detected gravitational wave source
• On the Rarity of X-Ray Binaries with Naked Helium Donors
• A Review of X-ray Observations of Supernova Remnants
• Gamma-ray burst host galaxies at low and high redshift
• Probing the Density in the Galactic Center Region: Wind-Blown Bubbles and High-Energy Proton Constraints
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• The Betelgeuse Project III: Merger Characteristics
• Inferring the progenitor mass-kinetic energy relation of stripped-envelope core-collapse supernovae from nebular spectroscopy
• Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925
• Stellar population synthesis models with a physically varying IMF
• Supernova and prompt gravitational-wave precursors to LIGO gravitational-wave sources and short-GRBs
• High Resolution X-ray Spectroscopy of G292.0+1.8/MSH 11-54
• The TRAPUM Small Magellanic Cloud pulsar survey with MeerKAT: I. Discovery of seven new pulsars and two Pulsar Wind Nebula associations
• Detailed Spectral Analysis of the Type Ib Supernova 1999dn. Paper I: Hydrogen-free Models
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
• Type IIP supernova SN 2016X in radio frequencies
• Early gray dust formation in the type IIn SN 2005ip
• Constraining the Low-Mass End of the Black Hole Mass Function and the Active Fraction of the Intermediate-mass Black Holes
• Herschel observations of dust around the high-mass X-ray binary GX 301-2
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• The EDGES measurement disfavors an excess radio background during the cosmic dawn
• SN 2020pvb: a Type IIn-P supernova with a precursor outburst
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
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• Luminous Blue Variables
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• Fragmentation of Primordial Filamentary Clouds under Far-Ultraviolet Radiation
• The explosion energy of the type IIP supernova SN 2013fs with a confined dense circumstellar shell
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• SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
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• Compact Object Formation and the Supernova Explosion Engine
• Signature of a massive rotating metal-poor star imprinted in the Phoenix stellar stream
• Multimessenger Universe with Gravitational Waves from Binaries
• Black Dwarf Supernova in the Far Future
• PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses
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• Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars
• Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299
• Study of X-ray emission from the S147 nebula by SRG/eROSITA: supernova-in-the-cavity scenario
• Numerical relativity simulations of black hole and relativistic jet formation
• TRAPUM search for pulsars in supernova remnants and pulsar wind nebulae -- I. Survey description and initial discoveries
• Formation and fate of low metallicity stars in IllustrisTNG50
• The formation of the stripped envelope type II b Supernova progenitors: Rotation, Metallicity and Overshooting
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• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• Black holes at cosmic dawn in the redshifted 21cm signal of HI
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Presolar grains
• A search for radio pulsars in five nearby supernova remnants
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
• Reassessing Dust's Role in Forming the CMB
• Investigating the observational properties of Type Ib supernova SN 2017iro
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems
• Cosmic Reionization and the First Nonlinear Structures in the Universe
• The effects of population III stars on the chemical and photometrical evolution of ellipticals
• The impact of precession on the observed population of ULXs
• Massive stars exploding in a He-rich circumstellar medium. XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc and 2024aej
• The Origin of the Possible Massive Black Hole in the Progenitor System of iPTF13bvn
• Circumstellar Na I and Ca II lines in type IIP supernovae and SN 1998S
• On the Progenitors of Core-Collapse Supernovae
• SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution
• Progenitors of Long-Duration Gamma-ray Bursts
• Optical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dld
• Is There a Universal Mass Function?
• Nebular C IV 1550 Imaging of the Metal-Poor Starburst Mrk 71: Direct Evidence of Catastrophic Cooling
• Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Accretion induced black hole spin up revised by numerical GR MHD simulations
• Thermal Regulation and the Star-Forming Main Sequence
• ORIGIN: Metal Creation and Evolution from the Cosmic Dawn
• Shock fronts in the long GRB031203 host galaxy
• The Lost Dwarfs of Centaurus A and the Formation of its Dark Globular Clusters
• Linking High- and Low-Mass Star Formation: Observation-Based Continuum Modelling and Physical Conditions
• Revealing the nature of the ULX and X-ray population of the spiral galaxy NGC 4088
• Unsupervised Transient Light Curve Analysis Via Hierarchical Bayesian Inference
• Formation of supermassive stars in the first stellar clusters: Dependence on the gas temperature
• Investigation of the Prompt SNe Ia progenitor nature through the analysis of the chemical composition of globular clusters and circumgalactic clouds
• A new model for the origin of very metal poor stars and their chemical composition
• Menus for Feeding Black Holes
• Stellar Evolution at Low Metallicity
• The formation of the first galaxies and the transition to low-mass star formation
• Determination of the angular momentum distribution of supernovae from gravitational wave observations
• Stellar Evolution in the Early Universe
• Beta decay and electron capture rates on manganese isotopes in astrophysical environments
• Multimessenger hierarchical triple merger gravitational-wave event pair GW190514-GW190521 inside AGN J124942.3 + 344929
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
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• The fate of rotating massive stars across cosmic times
• Moving inhomogeneous envelopes of stars
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• Helium-Star Models with Optically Thick Winds: Implications for the Internal Structures and Mass-Loss Rates of Wolf-Rayet Stars
• Gravitational Waves from Mirror World
• Black hole mass function shift in proto-stellar-clusters driven by gas accretion
• Quasi-star jets as unidentified gamma-ray sources
• Astrophysics with the Laser Interferometer Space Antenna
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• A new long gamma-ray burst formation pathway at solar metallicity
• High Velocity Runaway Binaries from Supernovae in Triple Systems
• Formation of the First Galaxies: Theory and Simulations
• Diffuse Neutrino Background from Magnetorotational Stellar Core Collapses
• The origins of low-luminosity supernovae: the case of SN 2016bkv
• Blue galaxies: modelling nebular He II emission in high redshift galaxies
• Are Supershells Powered by Multiple Supernovae? Modeling the Radio Pulsar Population Produced by OB Associations
• A Modified Initial Mass Function of the First Stars with Explodability Theory under Different Enrichment Scenarios
• Refining a relativistic, hydrodynamic solver: Admitting ultra-relativistic flows
• Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve
• Massive stars exploding in a He-rich circumstellar medium $-$ X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt
• Strange Dwarfs: a review on the (in)stability
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Hidden shock powering the peak of SN 2020faa
• The Origin and Detection of High-Redshift Supermassive Black Holes
• Nucleosynthesis in the accretion disks of Type II collapsars
• The effect of different eLISA-like configurations on massive black hole parameter estimation
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Fast and Not-so-Furious: Case Study of the Fast and Faint Type IIb SN 2021bxu
• First Stars. I. Evolution without mass loss
• X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
• The Red Supergiant Progenitor of the Type II Supernova 2024abfl
• Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback?
• IIb or not IIb: A Catalog of ZTF Kilonova Imposters
• Evolution of Massive Stars along the Cosmic History
• Exploring GRBs and supernovae connection: does a superluminous hypernova population exist?
• Small and Close-In Planets are Uncommon Around A-type Stars
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Recent LIGO-Virgo discoveries
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• The Unified Theory of Physics
• Stochastic Background of Gravitational Waves Generated by Eccentric Neutron Star Binaries
• The Cosmic Evolution of Gamma-Ray Burst Host Galaxies
• Core-collapse Supernovae and Gamma-ray Bursts in TMT Era
• MHD Interaction of Pulsar Wind Nebulae with SNRs and the ISM
• Effect of magnetic fields on the dynamics and gravitational wave emission of PPI-saturated self-gravitating accretion disks: simulations in full GR
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• Negative feedback effects on star formation history and cosmic reionization
• A theoretical color-velocity correlation for supernovae associated with gamma-ray bursts
• The Origin of the Metal-Poor Common Proper Motion Pair HD 134439/134440: Insights from New Elemental Abundances
• The Dawn of Black Holes
• Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
• A Pop III generated dust screen at z~16
• TRAPUM upper limits on pulsed radio emission for SMC X-ray pulsar J0058-7218
• Evolution of dwarf galaxy observable parameters
• Massive stars dying alone: the remote environment of SN 2010jp and its associated late-time source
• Impacts of the ${}^{12}\mathrm{C}{\left(\alpha ,\gamma \right)}^{16}\mathrm{O}$ reaction rate on ${}^{56}\mathrm{Ni}$ nucleosynthesis in pair-instability supernovae
• One of Everything: The Breakthrough Listen Exotica Catalog
• Detection of X-ray elongated emission from a ultraluminous X-ray source in the interacting pair of galaxies NGC 5953/5954
• Neutrino astrophysics : recent advances and open issues
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Accretion inside astrophysical objects : Effects of rotation and viscosity
• The Supernovae Analysis Application (SNAP)
• Globular cluster formation efficiencies from black-hole X-ray binary feedback
• Kickstarting Reionization with the First Black Holes: the effects of second-order perturbation theory in pre-reionization volumes
• Massive stars in their death-throes
• Post-explosion positive jet-feedback activity in inner ejecta of core collapse supernovae
• Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
• Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
• Modelling Thermonuclear X-ray Bursts on Accreting Neutron Stars
• Stellar evolution, SN explosion, and nucleosynthesis
• Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy
• Stellar-Mass Black Holes
• Quark-nova explosion inside a collapsar: application to Gamma Ray Bursts
• On the multiple supernova population of Arp 299: constraints on progenitor properties and host galaxy star formation characteristics
• The metallicity dependence of WR winds
• SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• Astrophysical black holes
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• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Growth and Feedback from the First Black Holes
• Thorne-Żytkow Objects
• TRAPUM pulsar and transient search in the Sextans A and B galaxies and discovery of background FRB 20210924D
• Search for high column density systems with gamma ray bursts
• Comparing the birth rate of stellar black holes in binary black hole mergers and long GRBs
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• Radio signals from early direct collapse black holes
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• New supernova remnant candidates in the LOFAR Two Metre Sky Survey
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• Searching for Pulsars, Magnetars, and Fast Radio Bursts in the Sculptor Galaxy using MeerKAT
• Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe
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• Galactic abundances as a relic neutrino detection scheme
• Investigating the dark matter minispikes with the gamma-ray signal from the halo of M31
• Star Formation for Predictive Primordial Galaxy Formation
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• Observed Consequences of Presupernova Instability in Very Massive Stars
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• SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
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• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• Mass loss and fate of the most massive stars
• The First Stars
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• Power-law Emission-line Wings and Radiation-Driven Superwinds in Local Lyman Continuum Emitters
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• Supernova dust for the extinction law in a young infrared galaxy at z = 1
• Parallelization of Kinetic Theory Simulations
• GRB160203A: an exploration of lumpy space
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• Neutrinos from Diffuse Supernova Background
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• On the emergence of a new instability during core-collapse of very massive stars
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• Electrically charged compact stars with an interacting quark equation of state
• First Stars. II. Evolution with mass loss
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• Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
• Nuclear astrophysics
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• Capability for detection of GW190521-like binary black holes with TianQin
• SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host
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• SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve
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• Radiative feedback on supermassive star formation: the massive end of the Population III initial mass function
• A Synthetic Population of Ultra-Luminous X-ray Sources: Optical-X-ray Correlation
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• Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey
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• Progenitors of Core-Collapse Supernovae
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