Observational clues to the progenitors of Type-Ia supernovae

Abstract

Type-Ia supernovae (SNe Ia) are important distance indicators, element factories, cosmic-ray accelerators, kinetic-energy sources in galaxy evolution, and endpoints of stellar binary evolution. It has long been clear that a SN Ia must be the runaway thermonuclear explosion of a degenerate carbon-oxygen stellar core, most likely a white dwarf (WD). However, the specific progenitor systems of SNe Ia, and the processes that lead to their ignition, have not been identified. Two broad classes of progenitor binary systems have long been considered: single-degenerate (SD), in which a WD gains mass from a non-degenerate star; and double-degenerate (DD), involving the merger of two WDs. New theoretical work has enriched these possibilities with some interesting updates and variants. We review the significant recent observational progress in addressing the progenitor problem. We consider clues that have emerged from the observed properties of the various proposed progenitor populations, from studies of their sites, pre- and post-explosion, from analysis of the explosions themselves, and from the measurement of event rates. The recent nearby and well-studied event, SN 2011fe, has been particularly revealing. The observational results are not yet conclusive, and sometimes prone to competing theoretical interpretations. Nevertheless, it appears that DD progenitors, long considered the underdog option, could be behind some, if not all, SNe Ia. We point to some directions that may lead to future progress.

to appear in Annual Reviews of Astronomy and Astrophysics, 2014. For near-final published version see http://www.annualreviews.org/doi/abs/10.1146/annurev-astro-082812-141031

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• The Multi-Epoch Nearby Cluster Survey: type Ia supernova rate measurement in z~0.1 clusters and the late-time delay time distribution
• Reflections on Reflexions: II. Effects of Light Echoes on the luminosity and spectra of Type Ia Supernovae
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• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
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• A common-envelope wind model for Type Ia supernovae (I): binary evolution and birth rate
• The double-degenerate model for the progenitors of type Ia supernovae
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• Thermonuclear detonations ensuing white dwarf mergers
• The Young and Nearby Normal Type Ia Supernova 2018gv: UV-Optical Observations and the Earliest Spectropolarimetry
• Binarity and beyond in A stars I. Survey description and first results of VLTI/GRAVITY observations of VAST targets with high Gaia-Hipparcos accelerations
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• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
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• Evidence for Sub-Chandrasekhar Mass Type Ia Supernovae from an Extensive Survey of Radiative Transfer Models
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• The metal content of the hot atmospheres of galaxy groups
• Three-Dimensional Simulation of Double-Detonations in the Double-Degenerate Model for Type Ia Supernovae and Interaction of Ejecta with a Surviving White Dwarf Companion
• Comprehensive models of novae at metallicity $Z=0.02$ and $Z=10^{-4}$
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• A New Catalogue of Galactic Novae: Investigation of the MMRD relation & Spatial Distribution
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• The Most Metal-poor Stars in the Magellanic Clouds are $r$-process Enhanced
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• An Excess of Mid-Infrared Emission from the Type Iax SN 2014dt
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• The Deepest Radio Observations of Nearby Type IA Supernovae: Constraining Progenitor Types and Optimizing Future Surveys
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• A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone can Explain Early-Excess Blue Flux in Some Type Ia Supernovae
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• No hot and luminous progenitor for Tycho's supernova
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• SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event
• The lowest of the low: discovery of SN 2019gsc and the nature of faint Iax supernovae
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• Supernovae and their host galaxies -- VII. The diversity of Type Ia supernova progenitors
• Infant-phase reddening by surface Fe-peak elements in a normal Type Ia Supernova
• A Carbon/Oxygen-dominated Atmosphere Days After Explosion for the "Super-Chandrasekhar" Type Ia SN 2020esm
• Double detonations: variations in Type Ia supernovae due to different core and He shell masses -- II: synthetic observables
• Early ultraviolet signatures from the interaction of Type Ia supernova ejecta with a stellar companion
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• Observations of SN 2015F suggest a correlation between the intrinsic luminosity of Type Ia supernovae and the shape of their light curves >900 days after explosion
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• Supernovae from direct collisions of white dwarfs and the role of helium shell ignition
• The Evolution of the Type Ia Supernova Luminosity Function
• Type Ia Supernovae: Colors, Rates, and Progenitors
• Hibernating black holes revealed by photometric mass functions
• The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way
• Explaining the early excess emission of the Type Ia supernova 2018oh by the interaction of the ejecta with disk-originated matter (DOM)
• Light Curves and Spectra from a Thermonuclear Explosion of a White Dwarf Merger
• The Oxygen Features in Type Ia Supernovae and the Implications for the Nature of Thermonuclear Explosions
• The luminous type Ia supernova 2022ilv and its early excess emission
• The circumstellar matter of supernova 2014J and the core-degenerate scenario
• Final Evolution and Delayed Explosions of Spinning White Dwarfs in Single Degenerate Models for Type Ia Supernovae
• Monte Carlo population synthesis of post-common-envelope white dwarf binaries and type Ia supernova rate
• JWST Low-Resolution MIRI Spectral Observations of SN~2021aefx: High-density Burning in a Type Ia Supernova
• Nebular spectroscopy of SN 2014J: Detection of stable nickel in near infrared spectra
• The fastest stars in the Galaxy
• On the maximum mass of magnetised white dwarfs
• No velocity-kicks are required to explain large-distance offsets of Ca-rich supernovae and short-GRBs
• Constraining axion-like particles using the white dwarf initial-final mass relation
• Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
• Observations of the Very Young Type Ia Supernova 2019np with Early-excess Emission
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• SN 2020kyg and the rates of faint Iax Supernovae from ATLAS
• Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs
• Getting to know Classical Novae with Swift
• ASASSN-15hy: an under-luminous, red 03fg-like type Ia supernova
• The effects of varying colour-luminosity relations on supernova science
• Optical and NIR observations of the nearby type Ia supernova SN 2014J
• Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397
• The formation of single neutron-stars from double white-dwarf mergers via accretion-induced collapse
• Neutrinos from type Ia supernovae: the deflagration-to-detonation transition scenario
• SN2002es-like Supernovae From Different Viewing Angles
• Do SN 2002cx-like and SN Ia-CSM objects share the same origin?
• Long-term evolution of double white dwarf binaries accreting through direct impact
• ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia
• Subdwarf B stars as possible surviving companions in Type Ia supernova remnants
• Variability, periodicity and contact binaries in WISE
• Neutrinos from type Ia supernovae: The gravitationally confined detonation scenario
• The single-degenerate model for the progenitors of accretion-induced collapse events
• Matching Globular Cluster Models to Observations
• The symbiotic recurrent nova V3890 Sgr: binary parameters and pre-outburst activity
• Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• The progenitors of type Ia supernovae in the semidetached binaries with red giant donors
• Search for Surviving Companions of Progenitors of Young LMC Type Ia Supernova Remnants
• The distant, galaxy cluster environment of the short GRB 161104A at $z\sim 0.8$ and a comparison to the short GRB host population
• Pan-Chromatic observations of the Recurrent Nova LMC 2009a (LMC 1971b)
• On the role of Type Ia supernovae in the second generation star formation in globular clusters
• Spatially Resolved Metal Loss from M31
• SN2019yvq Does Not Conform to SN Ia Explosion Models
• Optical and radio transients after the collapse of super-Chandrasekhar white dwarf merger remnants
• Nuclear processes in Astrophysics: Recent progress
• Modeling SNR G1.9+0.3 as a Supernova Inside a Planetary Nebula
• Identification of the feature that causes the I-band secondary maximum of a type Ia supernova
• Supernovae and their host galaxies - V. The vertical distribution of supernovae in disc galaxies
• Computational Tools for the Spectroscopic Analysis of White Dwarfs
• The interaction of Type Iax supernova ejecta with a helium companion star
• Two decades of optical timing of the shortest-period binary star system HM Cancri
• Supernova Rates and Luminosity Functions from ASAS-SN I: 2014--2017 Type Ia SNe and Their Subtypes
• Blue Large-Amplitude Pulsators: the Possible Surviving Companions of Type Ia Supernovae
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• The outcomes of carbon-oxygen white dwarfs accreting CO-rich material
• Constraining Type Ia Supernova Progenitor Scenarios with Extremely Late-time Photometry of Supernova SN 2013aa
• Trends in Nuclear Astrophysics
• A Self-Consistent Model for a Full Cycle of Recurrent Novae -- Wind Mass Loss Rate and X-Ray Luminosity
• Near-Chandrasekhar-Mass Type Ia Supernovae from the Double-Degenerate Channel
• A Significantly off-center Ni56 Distribution for the Low-Luminosity Type Ia Supernova SN 2016brx from the 100IAS survey
• Nebular spectra from Type Ia supernova explosion models compared to JWST observations of SN 2021aefx
• Nebular H$\alpha$ Limits for Fast Declining Type Ia Supernovae
• Sodium Absorption Systems toward SN Ia 2014J Originate on Interstellar Scales
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• A Luminous Peculiar Type Ia Supernova SN 2011hr: More Like SN 1991T or SN 2007if?
• Influence of a mass transfer stability criterion on double white dwarf populations
• From Out of the Blue: Swift Links 2002es-like, 2003fg-like, and Early-Time Bump Type Ia Supernovae
• Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud
• Discovery of the first resolved triple white dwarf
• Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae
• The CO White Dwarf + Intermediate Mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae
• Balmer-Dominated Shocks Exclude Hot Progenitors for Many Type Ia Supernovae
• Triple evolution: an important channel in the formation of type Ia supernovae
• A Black Hole - White Dwarf Compact Binary Model for Long Gamma-ray Bursts without Supernova Association
• Neutrinos from Type Ia and failed core-collapse supernovae at dark matter detectors
• Residual Carbon in Oxygen-Neon White Dwarfs and its Implications for Accretion-Induced Collapse
• The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies
• Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54
• Asymmetries in SN 2014J Near Maximum Light Revealed Through Spectropolarimetry
• Post-maximum near infrared spectra of SN 2014J: A search for interaction signatures
• Observational Constraints on the Common Envelope Phase
• Type Ia supernovae from non-accreting progenitors
• Mergers of Equal-Mass Binaries with Compact Object Companions from Mass Transfer in Triple Star Systems
• An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428
• Signatures of Bimodality in Nebular Phase Type Ia Supernova Spectra
• Sub-Chandrasekhar-mass detonations are in tension with the observed $t_0-M_{\text{Ni56}}$ relation of type Ia supernovae
• The most metal-rich stars in the universe: chemical contributions of low and intermediate mass asymptotic giant branch stars with metallicities between $0.04\le Z\le \mathrm{0.10.}$
• The ZTF-BTS Type Ia supernovae luminosity function is consistent with a single progenitor channel for the explosions
• The origin and evolution of the normal Type Ia SN 2018aoz with infant-phase reddening and excess emission
• Evolution of Magnetized White Dwarf Binaries to Type Ia Supernovae
• Constraining the origin and models of chemical enrichment in galaxy clusters using the Athena X-IFU
• Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process
• iPTF16abc and the population of Type Ia supernovae: Comparing the photospheric, transitional and nebular phases
• A simple and general method for solving detailed chemical evolution with delayed production of iron and other chemical elements
• Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics
• SN 2020sck: deflagration in a carbon-oxygen white dwarf
• Supernovae and their host galaxies -- VI. Normal Type Ia and 91bg-like supernovae in ellipticals
• The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia
• Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbv
• The Large Array Survey Telescope -- Science Goals
• Consistent extinction model for type Ia supernovae in Cepheid-based calibration galaxies and its impact on $H_0$
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Numerical simulations of high-energy flows in accreting magnetic white dwarfs
• Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
• Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
• Large-field CO(1--0) observations toward the Galactic historical supernova remnants: a large cavity around Tycho's supernova remnant
• Late-Time Observations of ASASSN-14lp Strengthen the Case for a Correlation between the Peak Luminosity of Type Ia Supernovae and the Shape of their Late-Time Light Curves
• Common envelope to explosion delay time of type Ia supernovae
• Evolution of Helium Star - White Dwarf Binaries Leading up to Thermonuclear Supernovae
• Cosmic-Ray Lithium Production at the Nova Eruption Followed by a Type Ia Supernova
• The Whisper of a Whimper of a Bang: 2400 Days of the Type Ia SN 2011fe Reveals the Decay of ${}^{55}$Fe
• Detection and classification of supernovae beyond z~2 redshift with the James Webb Space Telescope
• Gaia-Sausage-Enceladus star formation history as revealed by detailed elemental abundances
• Type Ia Supernovae and their Environment: Theory and Applications to SN 2014J
• Meeting the Challenges of Modeling Astrophysical Thermonuclear Explosions: Castro, Maestro, and the AMReX Astrophysics Suite
• An Intermediate Type Ia Supernova Between Normal And Super-Chandrasekhar
• Tycho's supernova: the view from {\it Gaia}
• The post-common-envelope X-ray binary nucleus of the planetary nebula NGC 2392
• The core-degenerate scenario for the progenitors of type Ia supernovae
• Investigation of the Progenitors of the Type Ia Supernovae Associated With the LMC Supernova Remnants 0505-67.9 and 0509-68.7
• An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-Degenerate Origin and Faint Hadronic Gamma-Rays
• Second generation star formation in globular clusters of different masses
• Merging of a CO WD and a He-rich white dwarf to produce a type Ia supernovae
• Prospects of Searching for Type Ia Supernovae with 2.5-m Wide Field Survey Telescope
• Constraints on the physical properties of Type Ia supernovae from photometry
• Surface and core detonations in rotating white dwarfs
• SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)
• Delayed Detonation Thermonuclear Supernovae With An Extended Dark Matter Component
• Type Ia Supernovae from wide white-dwarfs triples
• A 99-minute Double-lined White Dwarf Binary from SDSS-V
• Nebular Halpha emission in SN Ia 2016jae
• Cosmological constraint on Brans-Dicke Model
• The structure of a recent nova shell as observed by ALMA
• A magnetic white-dwarf accretion model for the anomalous X-ray pulsar 4U 0142+61
• Actinide crystallization and fission reactions in cooling white dwarf stars
• Nebular-Phase Spectra of Type Ia Supernovae from the Las Cumbres Observatory Global Supernova Project
• Spatially Resolved X-ray Spectroscopy of Kepler's Supernova Remnant: Distinct Properties of the Circumstellar Medium and the Ejecta
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Long-term evolution of surviving companion stars of Type Iax supernovae
• Can Kilonova Light curves be Standardized?
• Late-Time Observations of Type Ia Supernova SN 2014J with the Hubble Space Telescope Wide Field Camera 3
• SN 2012ij: A low-luminosity type Ia supernova and evidence for continuous distribution from 91bg-like explosion to normal ones
• Supernova 1604, Kepler's supernova, and its remnant
• One-Armed Spiral Instability in Double-Degenerate Post-Merger Accretion Disks
• SN 2014J at M82: I. A middle-class type Ia supernova by all spectroscopic metrics
• Production of Silicon on Mass Increasing White Dwarfs -- Possible Origin of High-Velocity-Features in Type Ia Supernovae
• SN 2015bp: adding to the growing population of transitional type Ia supernovae
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Discovery of $\sim$2200 new supernova remnants in 19 nearby star-forming galaxies with MUSE spectroscopy
• Late-Onset Circumstellar Medium Interactions are Rare: An Unbiased GALEX View of Type Ia Supernovae
• Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields
• Color-Magnitude Diagram Constraints on the Metallicities, Ages, and Star Formation History of the Stellar Populations in the Carina Dwarf Spheroidal Galaxy
• Searching for a Hypervelocity White Dwarf Companion: A Proper Motion Survey of SN 1006
• Progenitor constraints on the Type Ia supernova SN 2014J from Hubble Space Telescope H$\beta$ and [O III] observations
• Limits on a population of collisional-triples as progenitors of Type-Ia supernovae
• The Late-Time Light Curves of Type Ia Supernovae: Confronting Models with Observations
• The zenithal 4-m International Liquid Mirror Telescope: a unique facility for supernova studies
• The Way To a Double Degenerate: $\sim 15-20$ per cent of $1M_{\odot }\le M\le 8M_{\odot }$ Stars have a $M>1M_{\odot }$ Companion
• Rates and delay times of Type Ia supernovae in the helium-enriched main-sequence donor scenario
• Ultra wide black-hole - neutron star binaries as a possible source for gravitational waves and short gamma ray bursts
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Classifying Astronomical Transients Using Only Host Galaxy Photometry
• Attenuation of super-soft X-ray sources by circumstellar material
• Simulations of the symbiotic recurrent nova V407 Cyg. I. Accretion and shock evolutions
• Cosmic Type Ia SN rate and constraints on SN Ia progenitors
• Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
• Constraining the role of novae as progenitors of Type Ia Supernovae
• SNe Ia as a cosmological probe
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• The radial distribution of supernovae compared to star formation tracers
• An analysis of the spectroscopic signatures of layering in the ejecta of type Iax supernovae
• ZTF SN Ia DR2: The spectral diversity of Type Ia supernovae in a volume-limited sample
• Origin of high-velocity ejecta and early red excess emission in the infant Type Ia supernova 2021aefx
• Extreme close approaches in hierarchical triple systems with comparable masses
• The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event
• A Catalogue of Ultracompact Mass-Transferring White Dwarf Binaries
• Gas phase SiO in the circumstellar environment of the recurrent nova T Coronae Borealis
• The RR Lyrae Delay-Time Distribution: A Novel Perspective on Models of Old Stellar Populations
• Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
• The Gravitational Wave Emission of Double White Dwarf Coalescences
• On the nature of Fast Blue Optical Transients
• White dwarf - main sequence star collisions from wide triples in the field
• Exploration of Aspherical Ejecta Properties in Type Ia Supernova: Progenitor Dependence and Applications to Progenitor Classification
• A spectroscopic search for White Dwarf companions to 101 nearby M dwarfs
• On the [$\alpha$/Fe]-[Fe/H] relations in early-type galaxies
• Observational constraints on the origin of the elements. VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey
• A Polarization Sequence for Type Ia Supernovae?
• Probing the Progenitors of Type Ia Supernovae using Circumstellar Material Interaction Signatures
• Circumstellar properties of Type Ia supernovae from the helium star donor channel
• Constraining the Progenitor of the Type Ia Supernova SN 2012cg
• Possible Contribution of Magnetized White Dwarf Binaries to Type Ia Supernova Populations
• Rapidly evolving Galactic plane outbursts in NEOWISE: Revisiting the Galactic nova rate with the first all-sky search in the mid-infrared
• A feasibility study on the photometric detection of quiescent black hole X-ray binaries
• The Evolved Main-Sequence Channel: HST and LBT observations of CSS120422:111127+571239
• Nucleosynthesis signatures of neutrino-driven winds from proto-neutron stars: a perspective from chemical evolution models
• The Zadko Telescope: Exploring the transient Universe
• Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?
• Is the central binary system of the planetary nebula Henize 2-428 a Type Ia supernova progenitor?
• Understanding Type Ia supernovae through their U-band spectra
• Systematic errors on optical-SED stellar mass estimates for galaxies across cosmic time and their impact on cosmology
• Probing the efficiency of tidal synchronization in outspiralling double white dwarf binaries with LISA
• SN 2021fxy: Mid-Ultraviolet Flux Suppression is a Common Feature of Type Ia Supernovae
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• The interacting double white dwarf population with LISA; stochastic foreground and resolved sources
• Expected insights on type Ia supernovae from LISA's gravitational wave observations
• Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints
• From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
• Can the Helium-Enriched Main-Sequence Donor Scenario Hide Enough Hydrogen to Explain Type Ia Supernovae?
• Dust Formation and the Binary Companions of Supernovae
• Local Environments of Low-Redshift Supernovae
• Optical Observations of the Nearby Type Ia Supernova 2021hpr
• Asymmetric Expansion of the Fe ejecta in Kepler's Supernova Remnant
• The VISCACHA survey -- VIII. Chemical evolution history of Small Magellanic Cloud West Halo cluster
• The radial supernova remnant distribution in the Galaxy
• The two most recent thermonuclear supernovae in the Local Group: radio constraints on their progenitors and evolution
• An Eclipsing 47 minute Double White Dwarf Binary at 400 pc
• Hypervelocity binaries from close encounters with a SMBH-IMBH binary: orbital properties and diagnostics
• Comparing the Locations of Supernovae to CO (2-1) Emission in their Host Galaxies
• Constraints on the density distribution of type Ia supernovae ejecta inferred from late-time light-curve flattening
• Electromagnetic transients and gravitational waves from white dwarf disruptions by stellar black holes in triple systems
• Thirty Years of Radio Observations of Type Ia SN 1972E and SN 1895B: Constraints on Circumstellar Shells
• A study of Si II and S II features in spectra of Type Ia supernova
• SN 2015bq: A Luminous Type Ia Supernova with Early Flux Excess
• Star Formation and Chemical Enrichment in Protoclusters
• Physical Properties of the Host Galaxies of Ca-rich Transients
• Differentially Rotating White Dwarfs I: Regimes of Internal Rotation
• Reconciling Volumetric and Individual Galaxy Type Ia Supernova Rates
• The thermalization of $\gamma$-rays in radioactive expanding ejecta: A simple model and its application for Kilonovae and Ia SNe
• The first massive compact companion in a wide orbit around a hot subdwarf star
• Initial 56Ni Masses in Type Ia Supernovae
• On the relationship between Type Ia supernova luminosity and host-galaxy properties
• Metallicity Estimation of Core-Collapse Supernova HII Regions in Galaxies within 30 Mpc
• The effect of aspherical stellar wind of giant stars on the symbiotic channel of type Ia supernovae
• Detached Eclipsing Binaries in Compact Hierarchical Triples: Triple-lined systems BD+44 2258 and KIC 06525196
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
• Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299
• Constraining the Dimensionality of SN Ia Spectral Variation with Twins
• Photometric study of the late-time near-infrared plateau in Type Ia supernovae
• Elemental gas-phase abundances of intermediate redshift type Ia supernova star-forming host galaxies
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
• V445 Puppis -- Dustier than a Thousand Novae
• High-velocity feature as the indicator of the stellar population of Type Ia supernovae
• Observing the earliest moments of supernovae using strong gravitational lenses
• Supernova Remnants as Clues to Their Progenitors
• A Runaway Giant in the Galactic Halo
• Possible Circumstellar Interaction Origin of the Early Excess Emission in Thermonuclear Supernovae
• Properties of Type-Ia Supernova Light Curves
• The Impact of Resolution on Double-Detonation Models for Type Ia Supernovae
• Polarization signatures of the head-on collision model for Type Ia supernovae: How much asymmetry is too much?
• Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS
• SNGuess: A method for the selection of young extragalactic transients
• The aspherical explosions of the 03fg-like Type Ia supernovae 2021zny and 2022ilv revealed by polarimetry
• The supernova rate beyond the optical radius
• SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion
• Type Ia supernova ejecta-donor interaction: explosion model comparison
• SN 2017hpa: A Nearby Carbon-Rich Type Ia Supernova with a Large Velocity Gradient
• A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
• A possible surviving companion of the SN Ia in the Galactic SNR G272.2-3.2
• Non-thermal emission resulting from a supernova explosion inside an extragalactic jet
• Do Type Ia Supernovae Explode Inside Planetary Nebulae?
• Evolution of lithium in the disc of the Galaxy and the role of novae
• The Formation of Electron-capture Supernovae: A Review
• The Effects of Circumstellar Dust Scattering on the Light Curves and Polarizations of Type Ia Supernovae
• Physical conditions and element abundances in SN and GRB host galaxies at different redshifts
• Are Milky-Way-like galaxies like the Milky Way? A view from SDSS-IV/MaNGA
• The Hot Interstellar Medium
• Observations of A Fast-Expanding and UV-Bright Type Ia Supernova SN 2013gs
• Possible white dwarf progenitors of type Ia supernovae
• Locating the CSM Emission within the Type Ia Supernova Remnant N103B
• The Intrinsic Stochasticity of the ${}^{56}$Ni Distribution of Single-Degenerate Type Ia Supernovae
• White dwarf -- red giant star binaries as Type Ia supernova progenitors: with and without magnetic confinement
• Type Ia supernovae with and without blueshifted narrow Na I D lines - how different is their structure?
• Chemical enrichment in groups and clusters
• A closer look at non-interacting He stars as a channel for producing the old population of Type Ia supernovae
• On obliquely magnetized and differentially rotating stars
• A diverse, overlooked population of Type Ia supernovae exhibiting mid-infrared signatures of delayed circumstellar interaction
• Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
• Discovery of a ~30-Year-Duration Post-Nova Pulsating Supersoft Source in the Large Magellanic Cloud
• Dark Matter-Induced Baryonic Feedback in Galaxies
• An asymmetric explosion mechanism may explain the diversity of Si II line widths in Type Ia supernovae
• Electromagnetic signatures of white dwarf collisions in AGN discs
• SN 2016ije: An SN 2002es-like Type Ia Supernova Exploded in a Metal-poor and Low-surface Brightness Galaxy
• Multi-wavelength Observations of the 2015 Nova in the Local Group Irregular Dwarf Galaxy IC 1613
• Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
• A super-Eddington wind scenario for the progenitors of type Ia supernovae: binary population synthesis calculations
• Using ${}^{44}$Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors
• Chandra Fails to Detect X-ray Emission from Type Ia SN 2018fhw/ASASSN-18tb
• ZTF SN Ia DR2: Properties of the low-mass host galaxies of Type Ia supernovae in a volume-limited sample
• The Impact of the Environment of White Dwarf Mergers on Fast Radio Bursts
• Observational properties of a bright type Iax SN 2018cni and a faint type Iax SN 2020kyg
• Radio Observations of Six Young Type Ia Supernovae
• The accuracy of post-processing nucleosynthesis
• Simulating Kilonovae in the ΛCDM Universe
• ZTF SN Ia DR2: The secondary maximum in Type Ia supernovae
• Spatially Resolved Chandra Spectroscopy of Supernova Remnant DEM L71 in the Large Magellanic Cloud
• IIb or not IIb: A Catalog of ZTF Kilonova Imposters
• Why Are Peculiar Type Ia Supernovae More Likely to Show the Signature of a Single-degenerate Model?
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• Confronting double-detonation sub-Chandrasekhar models with the low-luminosity suppression of Type Ia supernovae
• Measurements of the Soft Gamma-ray Emission from SN2014J with Suzaku
• On the resonant detonation of sub-Chandrasekhar mass white dwarfs during binary inspiral
• Outside the Wall: Hydrodynamics of Type I Supernovae Interacting with a Partially Swept-Up Circumstellar Medium
• Comments on "Numerical Stability of Detonations in White Dwarf Simulations"
• Standardization of type Ia supernovae
• A spectroscopic quadruple as a possible progenitor of sub-Chandrasekhar Type Ia supernovae
• Thermonuclear (Type Ia) Supernovae and Progenitor Evolution
• On the relationship between metallicity distributions of globular clusters and of circumgalactic gas
• General relativistic pulsations of ultra-massive ZZ Ceti stars
• Synchrotron emission from double-peaked radio light curves of the symbiotic recurrent nova V3890 Sagitarii
• Revealing Double White Dwarf Mergers with Multi-messenger Signals
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
• The first phase of mass transfer in low-mass binaries: neither stable nor a common envelope
• Local two-dimensional simulations of the ignition of a helium shell detonation on a white dwarf by an impacting stream
• Merging White Dwarf Binaries Produce Type Ia Supernovae in Elliptical Galaxies
• LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
• Time-series spectroscopy of two candidate double degenerates in the open cluster NGC 6633
• Stellar evolution, SN explosion, and nucleosynthesis
• STag: Supernova Tagging and Classification
• Stellar evolution and modelling stars
• Building Blocks of the Milky Way's Accreted Spheroid
• A Semi-analytic Criterion for the Spontaneous Initiation of Carbon Detonations in White Dwarfs
• A Study of Magnetized White Dwarf + Helium Star Binary Evolution to Type Ia Supernovae
• The environments of Type Ia supernovae with different relative equivalent width of Si II feature in their spectra
• Incorporating Astrophysical Systematics into a Generalized Likelihood for Cosmology with Type Ia Supernovae
• Beyond binarity in A stars II. Disentangling the four stars in the vicinity of the triple HIP 87813 within the quintuple system HJ2814
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Highly reddened type Ia supernova SN 2004ab: another case of anomalous extinction
• Direct Analysis of the Broad-Line SN 2019ein: Connection with the Core-Normal SN 2011fe
• Discovery of a Proto-White Dwarf with a Massive Unseen Companion
• Off-centre ignition of sub-Chandrasekhar white dwarfs does not resolve the tension with the observed $t_0$-$M_{\mathrm{Ni}56}$ relation of type Ia supernovae
• Gravitational wave backgrounds from coalescing black hole binaries at cosmic dawn: an upper bound
• Core-collapse supernova from a possible progenitor star of 100 M${}_{\odot }$
• A comprehensive Gaia view of ellipsoidal and rotational red giant binaries
• Linking the properties of accreting white dwarfs with the ionization state of their ambient medium
• All known Type Ia supernovae models fail to reproduce the observed bolometric luminosity-width correlation
• New supernova remnant candidates in the LOFAR Two Metre Sky Survey
• Can helium envelopes change the outcome of direct white dwarf collisions?
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
• ZTF SN Ia DR2 follow-up: Exploring the origin of the Type Ia supernova host galaxy step through Si II velocities
• Past and future of the central double-degenerate core of Henize 2-428
• On the Time Variation of Dust Extinction and Gas Absorption for Type~Ia Supernovae Observed Through Non-uniform Interstellar Medium
• 3D Convective Urca Process in a Simmering White Dwarf
• Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
• Supernova environments in J-PLUS. Normalized Cumulative Rank distributions and stellar population synthesis, combining narrow- and broad-band filters
• Explaining supernova remnant G352.7-0.1 as a peculiar type Ia supernova inside a planetary nebula
• Do not forget the electrons: Extending moderately-sized nuclear networks for multidimensional hydrodynamic codes
• Degeneracy breakdown as a source of supernovae Ia
• Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Host Galaxy Effects in the Susy Model for Supernovae Ia
• X-Ray Observations of Type Ia Supernova 2018cqj
• High-energy Neutrinos from Stellar Explosions in Active Galactic Nuclei Accretion Disks
• The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation
• Type Ia supernovae SN 2013bz, PSN J0910+5003 and ASASSN-16ex: similar to 09dc-like?
• SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
• SN 2021hpr: A Normal Type Ia Supernova Showing Excess Emission in the Early Rising Phase
• Spectropolarimetry of the Type Ia SN 2019ein rules out significant global asphericity of the ejecta
• IK Pegasi and the Double-merger Path to Type Ia Supernovae
• SN 2017fgc: A Fast-Expanding Type Ia Supernova Exploded in Massive Shell Galaxy NGC 474
• Explosions in the Empty: A Survey of Transients in Local Void Galaxies
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Unveiling SN 2022eyw: A Bright Member of the Type Iax Supernova Subclass
• Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014
• AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary
• The Nova Synthetic Data Base: A Principal Component/AI Analysis of Novae Synoptic Spectra
• The Progenitor Systems of Classical Novae in M31
• The double detonation of a double degenerate system, from Type Ia supernova explosion to its supernova remnant
• Three-Dimensional Simulations of Type Ia Supernova Remnants I: Effects of a Main-Sequence Companion Star
• Search for gamma-ray emission from a galactic supernova with the anticoincidence system of SPI
• Estimating Transient Rates from Cosmological Simulations and BPASS
• Geodesics and Bending of Light around a BTZ Black Hole Surrounded by Quintessential Matter
• An imaging polarimetry survey of Type Ia supernovae: are peculiar extinction and polarization properties produced by circumstellar or interstellar matter?
• Detecting White Dwarf Binary Mergers with Gravitational Waves
• Discovery of a probable very fast extragalactic nova in a symbiotic binary
• Two Sites of r-Process Production Assessed on the Basis of the Age-tagged Abundances of Solar Twins
• Helium Accumulation and Thermonuclear Instabilities on Accreting White Dwarfs: From Recurring Helium Novae to Type Ia Supernovae
• SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart