Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions

Abstract

Nucleosynthesis, light curves, explosion energies, and remnant masses are calculated for a grid of supernovae resulting from massive stars with solar metallicity and masses from 9.0 to 120 solar masses. The full evolution is followed using an adaptive reaction network of up to 2000 nuclei. A novel aspect of the survey is the use of a one-dimensional neutrino transport model for the explosion. This explosion model has been calibrated to give the observed energy for SN 1987A, using several standard progenitors, and for the Crab supernova using a 9.6 solar mass progenitor. As a result of using a calibrated central engine, the final kinetic energy of the supernova is variable and sensitive to the structure of the presupernova star. Many progenitors with extended core structures do not explode, but become black holes, and the masses of exploding stars do not form a simply connected set. The resulting nucleosynthesis agrees reasonably well with the sun provided that a reasonable contribution from Type Ia supernovae is also allowed, but with a deficiency of light s-process isotopes. The resulting neutron star IMF has a mean gravitational mass near 1.4 solar masses. The average black hole mass is about 9 solar masses if only the helium core implodes, and 14 solar masses if the entire presupernova star collapses. Only ~10% of supernovae come from stars over 20 solar masses and some of these are Type Ib or Ic. Some useful systematics of Type IIp light curves are explored.

49 pages, 39 figures and 9 tables. Accepted to The Astrophysical Journal 26/1/2016

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• A Solar System formation analogue in the Ophiuchus star-forming complex
• Progenitor Mass Distribution for Core-Collapse Supernova Remnants in M31 and M33
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
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• The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
• Flavor Triangle of the Diffuse Supernova Neutrino Background
• Evidence from high mass X-ray binaries that Galactic WR components of WR+O binaries end their life with a supernova explosion
• LYRA III: The smallest Reionization survivors
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• The dusty aftermath of SN Hunt248: merger-burst remnant?
• The morphing of decay powered to interaction powered Type II supernova ejecta at nebular times
• Emission-line Wings Driven by Lyman Continuum in the Green Pea Analog Mrk 71
• Magnetar Powered Ordinary Type IIP Supernovae
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• The p-process in exploding rotating massive stars
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• Applications of Machine Learning to Predicting Core-collapse Supernova Explosion Outcomes
• Chemical abundances in Sgr A East: evidence for a Type Iax supernova remnant
• Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
• Shock Breakout in Dense Circumstellar Material with Application to PS1-13arp
• New \textsl{s}-process Mechanism in Rapidly-Rotating Massive Pop II Stars
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Shock breakouts from red supergiants: analytical and numerical predictions
• Magnetar-Powered Supernovae in Two Dimensions. II. Broad-Line Supernovae Ic
• Stellar Core-Merger-Induced Collapse: New Formation Pathways for Black Holes, Thorne-$\dot{\mathrm{Z}}$ytkow objects, Magnetars and Superluminous Supernovae
• Two-dimensional numerical study for magnetic field dependence of neutrino-driven core-collapse supernova models
• On the origin of nitrogen at low metallicity
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• Gaia's Detectability of Black Hole-Main Sequence Star Binaries Formed in Open Clusters
• A Critical Assessment of Turbulence Models for 1D Core-Collapse Supernova Simulations
• A solar-type star polluted by calcium-rich supernova ejecta inside the supernova remnant RCW 86
• Detailed X-Ray Mapping of the Shocked Ejecta and Circumstellar Medium in the Galactic Core-Collapse Supernova Remnant G292.0+1.8
• A Dark Energy Camera Search for Missing Supergiants in the LMC After the Advanced LIGO Gravitational Wave Event GW150914
• Nothing to see here: Failed supernovae are faint or rare
• Convection-Aided Explosions in One-Dimensional Core-Collapse Supernova Simulations I: Technique and Validation
• The synthesis of Ti44 and Ni56 in massive stars
• Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants
• Comparing simulated ${}^{26}$Al maps to gamma-ray measurements
• Progenitor mass and ejecta asymmetry of SN 2023ixf from nebular spectroscopy
• Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
• A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout
• Supernova-scope for the Direct Search of Supernova Axions
• Low luminosity Type II supernovae III. SN 2018hwm, a faint event with an unusually long plateau
• Nucleosynthesis Constraints on the Energy Growth Timescale of a Core-collapse Supernova Explosion
• The Energy Sources of Superluminous Supernovae
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• A Massive Star's Dying Breaths: Pulsating Red Supergiants and Their Resulting Type IIP Supernovae
• The Life Cycle of the Central Molecular Zone. II: Distribution of atomic and molecular gas tracers
• General Relativistic Neutrino-Driven Turbulence in One-Dimensional Core-Collapse Supernovae
• Constraining Compact Object Formation with 2M0521
• Detecting the Diffuse Supernova Neutrino Background in the future Water-based Liquid Scintillator Detector Theia
• Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• The Progenitor Age and Mass of the Black-Hole-Formation Candidate N6946-BH1
• Hydrodynamical modeling of the light curves of core collapse supernovae with HYPERION. I. The mass range 13-25 Msun, the metallicities -3<=[Fe/H]<=0 and the case of SN1999em
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
• A Comparison of Explosion Energies for Simulated and Observed Core-Collapse Supernovae
• Average opacity calculation for core-collapse supernovae
• The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?
• Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115
• The two promising scenarios to explode core collapse supernovae
• Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. II. Advanced modeling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernovae in the solar neighborhood
• Supernova 2018cuf: A Type IIP supernova with a slow fall from plateau
• The consequences of a nearby supernova on the early Solar System
• Second Generation Stars in Globular Clusters from Rapid Radiative Cooling of Pre-Supernova Massive Star Winds
• The IACOB project VIII. Searching for empirical signatures of binarity in fast-rotating O-type stars
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• A Sub-Solar Metallicity Progenitor for Cassiopeia A, the remnant of a Type IIb Supernova
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
• Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves
• The Origin of Cosmic Rays: How Their Composition Defines Their Sources and Sites, and the Processes of Their Mixing, Injection and Acceleration
• OGLE-2014-SN-073 as a fallback accretion powered supernova
• Supernovae Producing Unbound Binaries and Triples
• Formation and Evolution of Ultraluminous X-ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
• Progenitors and Explosion Properties of Supernova Remnants Hosting Central Compact Objects: I. RCW 103 Associated with the Peculiar Source 1E 161348-5055
• The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratio
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Reaction Rate Sensitivity of the Production of $\gamma$-ray Emitting Isotopes in Core-Collapse Supernova
• Monotonicity of the cores of massive stars
• SN 2015ba: A type IIP supernova with a long plateau
• The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies
• Post-explosion evolution of core-collapse supernovae
• Type II-P Supernova Progenitor Star Initial Masses and SN 2020jfo: Direct Detection, Light Curve Properties, Nebular Spectroscopy, and Local Environment
• A Transient Overcooling in the Early Universe? Clues from Globular Clusters Formation
• Type Ic Supernova of a 22 ${\text{M}}_{\odot }$ Progenitor
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• Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
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• Observational signature of circumstellar interaction and ${}^{56}$Ni-mixing in the Type II Supernova 2016gfy
• Helium giant stars as progenitors of rapidly fading Type Ibc supernovae
• The cosmic ray ionisation and $\gamma$-ray budgets of star-forming galaxies
• High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds
• Testing a one-dimensional prescription of dynamical shear mixing with a two-dimensional hydrodynamic simulation
• The circumstellar material around the Type IIP SN 2021yja
• A model for GN-z11: top-heavy stellar initial mass functions in forming galactic nuclei and ultra-compact dwarfs
• The Expansion of the Forward Shock of 1E 0102.2-7219 in X-rays
• A search for compact object companions to high mass function single-lined spectroscopic binaries in Gaia DR3
• Measurement of the X-ray proper motion in the south-east rim of RX J1713.7-3946
• Explosive nucleosynthesis with fast neutrino-flavor conversion in core-collapse supernovae
• Constraining the origin and models of chemical enrichment in galaxy clusters using the Athena X-IFU
• On the Progenitor of the Type Ic Supernova 2012fh
• Yellow Supergiants and Post-Red Supergiant Evolution in the Large Magellanic Cloud
• Inhomogeneous enrichment of radioactive nuclei in the Galaxy: Deposition of live Mn-53, Fe-60, Hf-182, and Pu-244 into deep-sea archives. Surfing the wave?
• Distribution and kinematics of 26Al in the Galactic disc
• Unveiling pure-metal ejecta X-ray emission in supernova remnants through their radiative recombination continuum
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• Powering luminous core collapse supernovae with jets
• On the maximum stellar rotation to form a black hole without an accompanying luminous transient
• An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
• The Nonstandard Properties of a "Standard" PWN: Unveiling the Mysteries of PWN G21.5-0.9 Using its IR and X-ray emission
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Shock Revival in Core-collapse Supernovae Assisted by Heavy Axion-like Particles
• The Late Time Optical Evolution of Twelve Core-Collapse Supernovae: Detection of Normal Stellar Winds
• A population of Type Ibc supernovae with massive progenitors; broad lightcurves not uncommon in (i)PTF
• Analysis of XMM-Newton Observations of Supernova Remnant W49B and Clues to the Progenitor
• Compact Object Candidates with K/M-dwarf Companions from LAMOST Low-resolution Survey
• A detailed look at the thermal and non-thermal X-ray emission from the Vela supernova remnant with SRG/eROSITA
• KSP-SN-2016kf: a long-rising H-rich Type II Supernova with unusually high ${}^{56}$Ni mass discovered in the KMTNet Supernova Program
• The 50-100pc scale parent stellar populations of type II supernovae and limitations of single star evolution models
• Chemical Evolution of Fluorine in the Milky Way
• LISA Detection of Binary Black Holes in the Milky Way Galaxy
• Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D
• The magnetar model of the superluminous supernova GAIA16apd and the explosion jet feedback mechanism (JFM)
• Estimating the core compactness of massive stars with Galactic supernova neutrinos
• SN 2016gsd: An unusually luminous and linear type II supernova with high velocities
• Progenitor Mass Distribution for 22 Historic Core-Collapse Supernovae
• The Galactic Underworld: The spatial distribution of compact remnants
• X-ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, its Wind Nebula and Hosting Supernova Remnant Kes 75
• The Impact of Initial-Final Mass Relations on Black Hole Microlensing
• Probing the Innermost Ejecta Layers in SNR Kes 75: Implications for the Supernova Progenitor
• Chemical enrichment in the cool core of the Centaurus cluster of galaxies
• Measuring the properties of $f-$mode oscillations of a protoneutron star by third generation gravitational-wave detectors
• How much H and He is "hidden" in SNe Ib/c? -- II. Intermediate-mass objects: a 22 M${}_{\odot }$ progenitor case study
• Tracer particles for core-collapse supernova nucleosynthesis: The advantages of moving backward
• Stability of the protoneutron stars toward black hole formation
• Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
• Magnetar-Driven Shock Breakout Revisited and Implications for Double-Peaked Type I Superluminous Supernovae
• 3D modeling from the onset of the SN to the full-fledged SNR: Role of an initial ejecta anisotropy on matter mixing
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• X-ray spectroscopy of the candidate AGN in Henize 2-10 and NGC 4178: Likely supernova remnants
• Proper Motion of the High-Velocity Pulsar in SNR MSH 15-56
• Chemical evolution of ${}^{26}$Al and ${}^{60}$Fe in the Milky Way
• Unveiling the Nature of SN 2011fh: a Young and Massive Star Gives Rise to a Luminous SN 2009ip-like Event
• SN 2023ixf -- an average-energy explosion with circumstellar medium and a precursor
• Diffuse neutrino background from past core-collapse supernovae
• SN 2018is: a low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Influence of macroclumping on type II supernova light curves
• Reducing Uncertainties in the Production of the Gamma Emitting Nuclei 26Al, 44Ti, and 60Fe in Core Collapse Supernovae by Using Effective Helium Burning Rates
• The giants that were born swiftly -- Implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
• A metallicity dependence on the occurrence of core-collapse supernovae
• Probing pre-supernova mass loss in double-peaked Type Ibc supernovae from the Zwicky Transient Facility
• Possible binary neutron star merger history of the primary of GW230529
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Evolution of the Black Hole Mass Function in Star Clusters from Multiple Mergers
• The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction
• SN 1961V: A Pulsational Pair-Instability Supernova
• An XMM-Newton X-ray View of Supernova Remnant W49B: Revisiting its Recombining Plasmas and Progenitor Type
• Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
• Pyroclastic Blowout: Dust Survival in Isolated versus Clustered Supernovae
• ASASSN-18am/SN 2018gk : An overluminous Type IIb supernova from a massive progenitor
• Binary progenitor systems for Type Ic supernovae
• Impact of late-time neutrino emission on the diffuse supernova neutrino background
• The jittering jets explosion mechanism (JJEM) in electron capture supernovae
• The radial distribution of supernovae compared to star formation tracers
• Tayler-Spruit dynamo in stably stratified rotating fluids: Application to proto-magnetars
• Quantifying the evidence against a mass gap between black holes and neutron stars
• Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
• Neutron stars formation and Core Collapse Supernovae
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Memory-triggered supernova neutrino detection
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches
• Effects of axions on Population III stars
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• A Consistent Modeling of Neutrino-driven Wind with Accretion Flow onto a Protoneutron Star and its Implications for ${}^{56}$Ni Production
• Predicted spatial and velocity distributions of ejected companion stars of helium accretion-induced thermonuclear supernovae
• Neutrino-dominated accretion flows: second nucleosynthesis factory in core-collapse supernovae and regulation of iron markets in galaxies
• Strongly lensed SN Refsdal: refining time delays based on the supernova explosion models
• Exploiting stellar explosion induced by the QCD phase transition in large-scale neutrino detectors
• Nucleosynthesis signatures of neutrino-driven winds from proto-neutron stars: a perspective from chemical evolution models
• Generating neutron-star magnetic fields: three dynamo phases
• The Masses of Supernova Remnant Progenitors in NGC 6946
• Explaining the ${}^{12}\text{C}{/}^{13}\text{C}$ ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars
• X-ray spectra of Sgr A East and diffuse X-ray background near the Galactic center
• Diffuse Neutrino Flux Based on the Rates of Core-collapse Supernovae and Black Hole Formation Deduced from a Novel Galactic Chemical Evolution Model
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae I: Spherically Symmetric Polytropic Models: Stability & Wind Emergence
• Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
• Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor
• Cobalt and copper abundances in 56 Galactic bulge red giants
• The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051
• The sub-critical illusion: synthetic Zeeman effect observations from galactic zoom-in simulations
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Disentangling the Black Hole Mass Spectrum with Photometric Microlensing Surveys
• Probing self-interacting sterile neutrino dark matter with the diffuse supernova neutrino background
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• How many explosions does one need? -- Quantifying supernovae in globular clusters from iron abundance spreads
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• SN 2018hna: Adding a Piece to the Puzzles of the Explosion of Blue Supergiants
• From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae I: Parameter Study of the Dependence on Jet Energetics
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Observing the Galactic Underworld: Predicting photometry and astrometry from compact remnant microlensing events
• Failed supernovae as a natural explanation for the binary black hole mass distribution
• Inferring Type II-P Supernova Progenitor Masses from Plateau Luminosities
• Ionization-Gasdynamic Simulations of Wind-Blown Nebulae around Massive Stars
• Spatially Resolved X-ray Study of Supernova Remnant G306.3$-$0.9 with Unusually High Calcium Abundance
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
• The Search for Failed Supernovae with the Large Binocular Telescope: N6946-BH1, Still No Star
• The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures
• Comparing Moment-Based and Monte Carlo Methods of Radiation Transport Modeling for Type II-Plateau Supernova Light Curves
• The Age Evolution of the Radio Morphology of Supernova Remnants
• Wolf-Rayet stars, black holes and the first detected gravitational wave source
• Disentangling the radio emission of the supernova remnant W51C
• Constraints on the density distribution of type Ia supernovae ejecta inferred from late-time light-curve flattening
• The Extremely Metal-Poor SN 2023ufx: A Local Analog to High-Redshift Type II Supernovae
• Comparing the Locations of Supernovae to CO (2-1) Emission in their Host Galaxies
• Fallback onto Kicked Neutron Stars and its Effect on Spin-Kick Alignment
• Galactic Population Synthesis of Radioactive Nucleosynthesis Ejecta
• Investigating episodic mass loss in evolved massive stars: II. Physical properties of red supergiants at subsolar metallicity
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
• Episodic mass loss in the very luminous red supergiant [W60] B90 in the Large Magellanic Cloud
• One Year of SN 2023ixf: Breaking Through the Degenerate Parameter Space in Light-Curve Models with Pulsating Progenitors
• The long-term influence of a magnetar power in stripped-envelope supernovae. Radiative-transfer modeling of He-star explosions from 1 to 10 years
• Untangling the Sources of Abundance Dispersion in Low-Metallicity Stars
• The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae
• Observational constraints on the origin of the elements. IX. 3D NLTE abundances of metals in the context of Galactic Chemical Evolution Models and 4MOST
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Parametric initial conditions for core-collapse supernova simulations
• Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299
• Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
• The Force Explosion Condition is Consistent with Spherically Symmetric CCSN Explosions
• Constraining the LyC escape fraction from LEGUS star clusters with SIGNALS HII region observations: A pilot study of NGC 628
• SN 2020cpg: an energetic link between type IIb and Ib supernovae
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• A global view of shocked plasma in the supernova remnant Puppis A provided by SRG/eROSITA
• Proposed Lunar Measurements of $r$-Process Radioisotopes to Distinguish Origin of Deep-sea 244Pu
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• Peculiar Supernovae
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• The Progenitor of the Vela Pulsar
• The Origin of the Possible Massive Black Hole in the Progenitor System of iPTF13bvn
• The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae II -- progenitor dependences --
• Isotopic ratios for C, N, Si, Al, and Ti in C-rich presolar grains from massive stars
• Formation and evolution of the local interstellar environment: combined constraints from nucleosynthetic and X-ray data
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae II: Comparisons with Abundances of Extremely Metal-Poor Galaxies and Constraints on Supernova Progenitors
• SN 2019nyk: A rapidly declining Type II supernova with early interaction signatures
• Near-critical supernova outflows and their neutrino signatures
• How does the stellar wind influence the radio morphology of a supernova remnant?
• On the limitations of H alpha luminosity as a star formation tracer in spatially resolved observations
• Progress in Nuclear Astrophysics of East and Southeast Asia
• The s process in massive stars, a benchmark for neutron capture reaction rates
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• The fate of rotating massive stars across cosmic times
• SN 2022acko: a low-luminosity SNe IIP with signs of early circumstellar interaction
• The Core-Collapse Supernova Explosion Mechanism
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• Low energy core collapse supernovae in the frame of the jittering jets explosion mechanism
• Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
• The initial mass-remnant mass relation for core collapse supernovae
• Progenitor constraint with circumstellar material for the magnetar-hosting supernova remnant RCW 103
• Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
• Investigation of the Prompt SNe Ia progenitor nature through the analysis of the chemical composition of globular clusters and circumgalactic clouds
• Nucleosynthesis Contribution of Neutrino-dominated Accretion Flows to the Chemical Evolution of Active Galactic Nuclei
• Quantum Black Hole Seismology II: Applications to Astrophysical Black Holes
• Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• Dark Age of Type II Supernova Remnants
• An Exploration of X-ray Supernova Remnants in the Milky Way and Nearby Galaxies
• Radiative-transfer models for dusty Type II supernovae
• On the Formation of SS433
• Prospects for Time-Domain and Multi-Messenger Science with eXTP
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae II: Rotation and Turbulence
• Black hole mass function shift in proto-stellar-clusters driven by gas accretion
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Theoretical Distributions of Short-Lived Radionuclides for Star Formation in Molecular Clouds
• Fermi-LAT Gamma-ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud
• O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
• Sensitivity of multi-PMT Optical Modules in Antarctic Ice to Supernova Neutrinos of MeV energy
• Natal kicks of compact objects
• SN 2018gk Revisited: the Photosphere, the Central Engine, And the Putative Dust
• Weighing stars from birth to death: mass determination methods across the HRD
• Gravitational Microlensing Event Statistics for the Zwicky Transient Facility
• Modelling light curves of bipolar core collapse supernovae from the equatorial plane
• The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• Failed Supernova Remnants
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
• Fast and Not-so-Furious: Case Study of the Fast and Faint Type IIb SN 2021bxu
• The population of Galactic supernova remnants in the TeV range
• Dancing with invisible partners: Three-body exchanges with primordial black holes
• A survey of extremely metal-poor gas at cosmic noon: evidence of elevated [O/Fe]
• Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole
• Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors
• Mass Distribution of Binary Black Hole Mergers from Young and Old Dense Star Clusters
• IIb or not IIb: A Catalog of ZTF Kilonova Imposters
• Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
• Investigating episodic mass loss in evolved massive stars: III. Spectroscopy of dusty massive stars in three northern galaxies
• Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
• A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
• SPI Analysis and Abundance Calculations of DEM L71, and Comparison to SN explosion Models
• Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
• Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• Post-explosion positive jet-feedback activity in inner ejecta of core collapse supernovae
• Surrogate models for lightcurves and photosphere properties of Type II supernovae
• New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling
• Pre-explosion, explosion, and post-explosion jets in supernova SN 2019zrk
• Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network
• Binary stellar evolution yields in galactic chemical evolution calculations
• Properties of Thorne-Zytkow object explosions
• Triangulating Black Hole Forming Stellar Collapses through Neutrinos
• Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC
• X-raying the Birth of Binary Neutron Stars and Neutron Star-Black Hole Binaries
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Scalar Gravitational Wave Signals from Core Collapse in Massive Scalar-Tensor Gravity with Triple-Scalar Interactions
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Revisiting the abundance pattern and charge-exchange emission in the M82 centre
• Evolution of eccentric high-mass X-ray binaries. The case of GX 301-2
• A mixed helium-oxygen shell in some core-collapse supernova progenitors
• Mapping Progenitors of Binary Black Holes and Neutron Stars with Binary Population Synthesis
• Fundamental limits to orbit reconstruction due to non-conservation of stellar actions in a Milky Way-like simulation
• XRISM Observations of Cassiopeia A: Overview, Atomic Data, and Spectral Models
• Black holes formed by direct collapse: observational evidences
• Stellar progenitors of black holes: insights from optical and infrared observations
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• Revisiting the Galactic Winds in M82 II: Development of Multiphase Outflows in Simulations
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• The environment of TeV halo progenitors
• Constraints on Explosion Timescale of Core-Collapse Supernovae Based on Systematic Analysis of Light Curves
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• The K supergiant runaway star HD 137071
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• Uncovering the neutrino mass ordering with the next galactic core-collapse supernova neutrino burst using water Cherenkov detectors
• Modeling the light curve of Type IIn-P SN 2005cl with red supergiant progenitors featuring pre-SN ourbursts
• Production of heavy $\alpha$-elements and ${}^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
• Testing the presence of a dormant black hole inside HR 6819
• SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
• Core-collapse supernova parameter estimation with the upcoming Vera C. Rubin Observatory
• Spherically Symmetric Accretion onto a Compact Object through a Standing Shock: The Effects of General Relativity in the Schwarzschild Geometry
• Rapid decline in the lightcurves of luminous supernovae by jet-driven bipolar explosions
• SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
• Core-Collapse Supernovae: From Neutrino-Driven 1D Explosions to Light Curves and Spectra
• Typing supernova remnant G352.7$-$0.1 using XMM-Newton X-ray observations
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Radioactive Decay
• Fast Transients from Magnetic Disks Around Non-Spinning Collapsar Black Holes
• Neutrinos from Diffuse Supernova Background
• A Large-scale Approach to Modelling Molecular Biosignatures: The Diatomics
• Individual Neutrino Masses From a Supernova
• The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
• Power-law Emission-line Wings and Radiation-Driven Superwinds in Local Lyman Continuum Emitters
• Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
• New experimental ${}^{23}$Na($\alpha ,p$)${}^{26}$Mg Reaction Rate for Massive Star and Type-Ia Supernova models
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
• The influence of rotation and metallicity on the explodability of massive stars
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Accurate Determination of Chemical Abundances near a Supermassive Black Hole
• PGIR 20eid (SN2020qmp): A Type IIP Supernova at 15.6 Mpc discovered by the Palomar Gattini-IR survey
• The aluminium-26 distribution in a cosmological simulation of a Milky Way-type Galaxy
• XMM-Newton Observations of the High Temperature Plasma in the Large Magellanic Cloud Supernova Remnant N132D
• On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis
• Evolution of proto-neutron stars to pulsars, magnetars and central compact objects
• Discovery of a 310-day Period from the Enshrouded Massive System NaSt1 (WR 122)
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• Cosmic Radioactivity and Galactic Chemical Evolution
• Self-consistent Conditions for ${}^{26}$Al Injection into Protosolar Disk from a Nearby Supernova
• Successful $\nu p$-process in neutrino-driven outflows in core-collapse supernovae
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• The Formation of Globular Clusters as a Case of Overcooling
• Distinguishing Dirac and Majorana Neutrinos: Resonant Spin-Flavor Precession of GeV-Scale Astrophysical Transients
• Constraining Black Hole Natal Kicks with Astrometric Microlensing
• New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State
• Chemical enrichment of ICM within the A3266 cluster I: radial profiles
• The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases
• SN 2017ati: A luminous type IIb explosion from a massive progenitor
• An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing
• The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants
• Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness
• Dynamical double black holes and their host cluster properties
• Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad
• Massive stars evolution: feedbacks in low-Z environment
• Astrometric microlensing probes of the isolated neutron star population with Roman
• QED V: Variations in metal loading of galactic winds with element nucleosynthetic origin
• Direct Detection of Type II-P Supernova Progenitors with the $\text{Euclid}$ and CSST Surveys
• Evolution of action-space coherence in a Milky Way-like simulation
• Ranking Theoretical Supernovae Explosion Models from Observations of the Intracluster Gas
• A New Versatile Code for Gamma-Ray Monte-Carlo Radiative Transfer
• Electron-capture Supernova Candidates from Light Curves: Implications for Their Progenitors and Explosion Properties
• Chandra and XMM-Newton X-ray Study on the Core-collapse Supernova Remnant N63A in an H II Region
• The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\mathrm{X}}$--$T$ relation of early-type galaxies
• Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole?
• Mass measurements of the double neutron star system PSR J0641+0448
• Formation of black holes from He stars
• SNR G292.0+1.8: A Remnant of a Low-Mass Progenitor Stripped-Envelope Supernova
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• Progenitor and Close-In Circumstellar Medium of Type II Supernova 2020fqv from High-Cadence Photometry and Ultra-Rapid UV Spectroscopy
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase