The single degenerate channel for the progenitors of type Ia supernovae

Abstract

We have carried out a detailed study of one of the most popular evolutionary channels for the production of Type Ia supernova (SN Ia) progenitors, the semi-degenerate channel (CO+MS), where a carbon/oxygen (CO) white dwarf (WD) accretes matter from an unevolved or slightly evolved non-degenerate star until it reaches the Chandrasekhar mass limit. Employing Eggleton's stellar evolution code and adopting the prescription of Hachisu et al. (1999) for the accretion efficiency, we have carried out full binary evolution calculations for about 2300 close WD binary systems and mapped out the initial parameters in the orbital period -- secondary mass ($P$--$M_2$) plane (for a range of WD masses) which lead to a successful Type Ia supernova. We obtained accurate, analytical fitting formulae to describe this parameter range which can be used for binary population synthesis (BPS) studies. The contours in the $P$--$M_2$ plane differ from those obtained by Hachisu et al. (1999) for low-mass CO WDs, which are more common than massive CO WDs. We show that white dwarfs with a mass as low as $0.67M_{\odot }$ can accrete efficiently and reach the Chandrasekhar limit. We have implemented these results in a BPS study to obtain the birthrates for SNe Ia and the evolution of birthrates with time of SNe Ia for both a constant star formation rate and a single star burst. The birthrates are somewhat lower than (but comparable to) those inferred observationally.

10 pages, 14 figures, submitted to MNRAS

References in corpus (15)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The origin of sdB stars (II)
• Approximate input physics for stellar modelling
• A Wide Symbiotic Channel to Type Ia Supernovae
• Type Ia Supernovae: Influence of the Initial Composition on the Nucleosynthesis, Light Curves, Spectra and Consequences for the Determination of Omega_M & Lambda
• A New Evolutionary Path to Type Ia Supernovae: Helium-Rich Super-Soft X-Ray Source Channel
• Supernovae Rates: A Cosmic History
• Low and intermediate-mass close binary evolution and the initial - final mass relation
• Thermal Timescale Mass Transfer and the Evolution of White Dwarf Binaries
• Type Ia Supernovae: An Examination of Potential Progenitors and the Redshift Distribution
• Cygnus X-2, super-Eddington mass transfer, and pulsar binaries
• Cygnus X-2: the Descendant of an Intermediate-Mass X-Ray Binary
• Images of an equatorial outflow in SS433
• Type Ia Supernovae in semi-detached binary systems

Cited by in corpus (288)

• Common Envelope Evolution: Where we stand and how we can move forward
• Observational clues to the progenitors of Type-Ia supernovae
• Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
• The Evolution of Compact Binary Star Systems
• Progenitors of type Ia supernovae
• Hubble Residuals of Nearby Type Ia Supernovae Are Correlated with Host Galaxy Masses
• PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor
• Rates and Delay Times of Type Ia Supernovae
• Supernova Type Ia progenitors from merging double white dwarfs: Using a new population synthesis model
• Type-Ia supernova rates and the progenitor problem, a review
• The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models
• Helium-ignited violent mergers as a unified model for normal and rapidly declining Type Ia Supernovae
• A Compact Degenerate Primary-Star Progenitor of SN 2011fe
• The delay-time distribution of type-Ia supernovae from Sloan II
• The rates of Type Ia Supernovae. I. Analytical Formulations
• Theoretical uncertainties of the type Ia supernova rate
• Delay Time Distribution Measurement of Type Ia Supernovae by the Subaru/XMM-Newton Deep Survey and Implications for the Progenitor
• Double-detonation supernovae of sub-Chandrasekhar mass white dwarfs
• Thermal Stability of White Dwarfs Accreting Hydrogen-rich Matter and Progenitors of Type Ia Supernovae
• On the evolution of rapidly rotating massive white dwarfs towards supernovae or collapses
• 3D deflagration simulations leaving bound remnants: a model for 2002cx-like Type Ia supernovae
• The supernova delay time distribution in galaxy clusters and implications for Type-Ia progenitors and metal enrichment
• Helium star donor channel for the progenitors of type Ia supernovae
• A binary model for the UV-upturn of elliptical galaxies (MNRAS version)
• Abundance stratification in Type Ia supernovae - I. The case of SN 2002bo
• The Progenitors of Type Ia Supernovae
• On the Progenitors of Type Ia Supernovae
• EVLA Observations Constrain the Environment and Progenitor System of Type Ia Supernova 2011fe
• Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• Single-degenerate type Ia supernovae without hydrogen contamination
• Nearby Supernova Rates from the Lick Observatory Supernova Search. IV. A Recovery Method for the Delay Time Distribution
• Type Ia Supernova Explosions in Binary Systems: A Review
• Mass accumulation efficiency in helium shell flashes for various white dwarf masses
• Type Ia supernova bolometric light curves and ejected mass estimates from the Nearby Supernova Factory
• Evolution towards and beyond accretion-induced collapse of massive white dwarfs and formation of millisecond pulsars
• Young and Massive Binary Progenitors of Type Ia Supernovae and Their Circumstellar Matter
• Subaru high-resolution spectroscopy of Star G in the Tycho supernova remnant
• Early radio and X-ray observations of the youngest nearby type Ia supernova PTF11kly (SN 2011fe)
• Mass-accreting white dwarfs and type Ia supernovae
• The supernova rate and delay time distribution in the Magellanic Clouds
• No X-rays from the very nearby Type Ia SN2014J: constraints on its environment
• Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2
• The Effect of Different Type Ia Supernova Progenitors on Galactic Chemical Evolution
• The impact of type Ia supernovae on main sequence binary companions
• The Evolution of Compact Binary Star Systems
• The Type Ia Supernova Rate at z ~0.5 from the Supernova Legacy Survey
• Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
• i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
• Binary Population Synthesis
• The delay time distribution of type Ia supernovae: a comparison between theory and observation
• The single-degenerate channel for the progenitor of type Ia supernovae with different metallicities
• The nucleosynthetic history of elements in the Galactic disk: [X/Fe] - age relations from high-precision spectroscopy
• On type Ia supernovae and the formation of single low-mass white dwarfs
• The progenitors of Type Ia supernovae with long delay times
• Evolving to Type Ia Supernovae with Short Delay Times
• Type IA supernovae from very long delayed explosion of core - WD merger
• PopCORN: Hunting down the differences between binary population synthesis codes
• A census of symbiotic stars in the 2MASS, WISE and Gaia surveys
• Formation of Extremely Low-mass White Dwarfs in Double Degenerates
• Constraints on the Progenitor System of the Type Ia Supernova 2014J from Pre-Explosion Hubble Space Telescope Imaging
• Companion stars of Type Ia supernovae and hypervelocity stars
• A single-degenerate model for the progenitor of the Type Ia supernova 2002ic
• The impact of Type Ia supernova explosions on helium companions in the Chandrasekhar-mass explosion scenario
• Explaining the type Ia supernova PTF 11kx with a violent-prompt merger scenario
• Producing type Iax supernovae from a specific class of helium-ignited WD explosions?
• The i-process yields of rapidly-accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parameterizations from 3D hydrodynamics simulations
• The Masses and Accretion Rates of White Dwarfs in Classical and Recurrent Novae
• Searching for a Companion Star of Tycho's Type Ia Supernova with Optical Spectroscopic Observations
• Shortest Recurrence Periods of Novae
• Progenitors of Type Ia Supernovae: Binary Stars with White Dwarf Companions
• Single Degenerate Models for Type Ia Supernovae Progenitor's Evolution and Nucleosythesis Yields
• The many sides of RCW 86: a type Ia supernova remnant evolving in its progenitor's wind bubble
• Companion Stars of Type Ia Supernovae
• Supernovae Sparked By Dark Matter in White Dwarfs
• On the progenitors of super-Chandrasekhar mass type Ia supernovae
• He-accreting carbon-oxygen white dwarfs and type Ia supernovae
• On the fraction of intermediate-mass close binaries that explode as type-Ia supernovae
• Modelling the circumstellar medium in RS Ophiuchi and its link to Type Ia supernovae
• The C-flash and the ignition conditions of type Ia supernovae
• The fraction of type Ia supernovae exploding inside planetary nebulae (SNIPs)
• A hot subdwarf-white dwarf super-Chandrasekhar candidate supernova Ia progenitor
• New constraints on SN Ia progenitor models
• Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution spectroscopic observations
• A comprehensive progenitor model for SNe Ia
• Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T
• ASASSN-18tb: A Most Unusual Type Ia Supernova Observed by TESS and SALT
• Detectability of ultra-compact X-ray binaries as LISA sources
• Expanding molecular bubble surrounding Tycho's supernova remnant (SN 1572) observed with IRAM 30 m telescope: evidence for a single-degenerate progenitor
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
• The astrophysical science case for a decihertz gravitational-wave detector
• Single degenerate supernova type Ia progenitors
• A machine learning approach for identification and classification of symbiotic stars using 2MASS and WISE
• Hierarchical Growth and Cosmic Star Formation: Enrichment, Outflows and Supernova Rates
• The rates of Type Ia Supernovae. II. Diversity of events at low and high redshift
• Binary Stars in the New Millennium
• Constraints on SN Ia progenitor time delays from high-z SNe and the star formation history
• Primordial Binary Evolution and Blue Stragglers
• New approaches to SNe Ia progenitors
• Tidally enhanced stellar wind: a way to make the symbiotic channel to Type Ia supernova viable
• Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
• Post-common envelope binaries from SDSS - XVI. Long orbital period systems and the energy budget of CE evolution
• Type Ia Supernovae inside Planetary Nebulae: Shaping by Jets
• Where are the double-degenerate progenitors of type Ia supernovae?
• 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
• Evolution of Post-Impact Companion Stars in SN Ia Remnants within the Single-Degenerate Scenario
• i-Process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-Peak Neutron-Capture Elements
• The number of progenitors in the core - degenerate scenario for type Ia supernovae
• Accelerating Composite Dark Matter Discovery with Nuclear Recoils and the Migdal Effect
• Constraining the double-degenerate scenario for Type Ia supernovae from merger ejected matter
• The birth rate of SNe Ia from hybrid CONe white dwarfs
• Pulsating reverse detonation models of Type Ia supernovae. II: Explosion
• The helium star donor channel for the progenitors of type Ia supernovae with different metallicities
• The hybrid CONe WD + He star scenario for the progenitors of type Ia supernovae
• The explosion of supernova 2011fe in the frame of the core-degenerate scenario
• Pulsating reverse detonation models of Type Ia supernovae. I: Detonation ignition
• Evolving to type Ia supernovae with long delay time
• White dwarf-main sequence binaries from LAMOST: the DR5 catalogue
• Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
• The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4
• Helium star evolutionary channel to super-Chandrasekhar mass type Ia supernovae
• The Large-Scale Environments of Type Ia Supernovae: Evidence for a Metallicity Bias in the Rate or Luminosity of Prompt Ia Events
• On the evolution of rotating accreting white dwarfs and type Ia supernovae
• The rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario
• Variable H$\alpha$ Emission in the Nebular Spectra of the Low-Luminosity Type Ia SN2018cqj/ATLAS18qtd
• Upper limit for circumstellar gas around the Type Ia SN 2000cx
• Predicting the amount of hydrogen stripped by the supernova explosion for SN 2002cx-like SNe Ia
• Dust Formation in the Ejecta of Common Envelope Systems
• Population synthesis of accreting white dwarfs: II. X-ray and UV emission
• The response of a helium white dwarf to an exploding type Ia supernova
• Keck Observations of the Young Metal-Poor Host Galaxy of the Super-Chandrasekhar-Mass Type Ia Supernova SN 2007if
• Multi-wavelength Light Curve Model of the One-year Recurrence Period Nova M31N 2008-12a
• Supernova progenitors and iron density evolution from SN rate evolution measurements
• The violent white dwarf merger scenario for the progenitors of type Ia supernovae
• The radial distribution of type Ia supernovae in early-type galaxies: implications for progenitor scenarios
• Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
• Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae
• How old are SN Ia Progenitor Systems? New Observational Constraints on the Distribution of Time Delays from GALEX
• On the Lira law and the nature of extinction towards Type Ia Supernovae
• Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA
• The origin of abundance gradients in the Milky Way: the predictions of different models
• Smoothed Particle Hydrodynamics simulations of the core-degenerate scenario for Type Ia supernovae
• Supernovae and their host galaxies -- VII. The diversity of Type Ia supernova progenitors
• Pre-explosion companion stars in Type Iax supernovae
• Neutronization During Carbon Simmering In Type Ia Supernova Progenitors
• Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
• Early ultraviolet signatures from the interaction of Type Ia supernova ejecta with a stellar companion
• Some constraints on the lower mass limit for double-degenerate progenitors of Type Ia supernovae
• Probing thermonuclear supernova explosions with neutrinos
• The circumstellar matter of supernova 2014J and the core-degenerate scenario
• Type Ia Supernovae: Colors, Rates, and Progenitors
• The bifurcation periods in low-mass X-ray binaries: the effect of magnetic braking and mass loss
• Formation of Millisecond Pulsars with Low-Mass Helium White Dwarf Companions in Very Compact Binaries
• Companion stars of Type Ia supernovae and single low-mass white dwarfs
• Galactic and Cosmic Type Ia SN rates: is it possible to impose constraints on SNIa progenitors?
• Super-Eddington wind scenario for the progenitors of type Ia supernovae: Accreting He-rich matter onto white dwarfs
• The white dwarf binary pathways survey V. The Gaia white dwarf plus AFGK binary sample and the identification of 23 close binaries
• Distribution of ${}^{56}$Ni Yields of Type Ia Supernovae and its Implication for Progenitors
• Early UV emission from disk-originated matter (DOM) in type Ia supernovae in the double degenerate scenario
• Do SN 2002cx-like and SN Ia-CSM objects share the same origin?
• A likely candidate of type Ia supernova progenitors: the X-ray pulsating companion of the hot subdwarf HD 49798
• LAMOST J0140355+392651: An evolved cataclysmic variable donor transitioning to become an extremely low mass white dwarf
• The single-degenerate model for the progenitors of accretion-induced collapse events
• 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
• Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs
• The Evolution of Helium Star Plus Carbon-Oxygen White Dwarf Binary Systems and Implications for Diverse Stellar Transients and Hypervelocity Stars
• The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters
• 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
• Constraining the spin-down timescale of the white-dwarf progenitors of Type Ia supernovae
• Theoretical cosmic Type Ia supernova rates
• The interaction of Type Iax supernova ejecta with a helium companion star
• A Self-Consistent Model for a Full Cycle of Recurrent Novae -- Wind Mass Loss Rate and X-Ray Luminosity
• White dwarf-main sequence binaries identified from the LAMOST pilot survey
• Accreting CO material onto ONe white dwarfs towards accretion-induced collapse
• A Super-Eddington Wind Scenario for the Progenitors of Type Ia Supernovae
• The CO White Dwarf + Intermediate Mass/Massive Star Binary Evolution: Possible Merger Origins for Peculiar Type Ia and II Supernovae
• General Relativistic White Dwarfs and Their Astrophysical Implications
• Spatially Resolved RGS Analysis of Kepler's Supernova Remnant
• Revisiting Common Envelope Evolution -- A New Semi-Analytic Model for N-body and Population Synthesis Codes
• An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428
• Signatures of Bimodality in Nebular Phase Type Ia Supernova Spectra
• The structure and stability of massive hot white dwarfs
• SN 2020sck: deflagration in a carbon-oxygen white dwarf
• Progenitors of Supernovae Type Ia and Chemical Enrichment in Hydrodynamical Simulations -I. The Single Degenerate Scenario
• The birth rate of subluminous and overluminous type Ia supernovae
• Birthrates and delay times of Type Ia supernovae
• Wind-Driven Evolution of White Dwarf Binaries to Type Ia Supernovae
• WD+RG systems as the progenitors of Type Ia supernovae
• The Swift Bulge Survey: optical and near-IR follow-up featuring a likely symbiotic X-ray binary & a focused wind CV
• Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
• Type Ia Supernova Remnants: Shaping by Iron Bullets
• The Spin Evolution of Fast-Rotating, Magnetized Super-Chandrasekhar White Dwarfs in the Aftermath of White Dwarf Mergers
• The X-ray/radio and UV luminosity expected from symbiotic systems as the progenitor of SNe Ia
• Common envelope to explosion delay time of type Ia supernovae
• Exploring the Carbon Simmering Phase: Reaction Rates, Mixing, and the Convective Urca Process
• Companion Stars of Type Ia supernovae with different metallicities
• CI Aql: a Type Ia supernova progenitor?
• Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
• Investigation of the Progenitors of the Type Ia Supernovae Associated With the LMC Supernova Remnants 0505-67.9 and 0509-68.7
• What sodium absorption lines tell us about type Ia supernovae
• The core-degenerate scenario for the progenitors of type Ia supernovae
• Merging of a CO WD and a He-rich white dwarf to produce a type Ia supernovae
• Population Synthesis of Millisecond X-ray Pulsars
• Shortest Recurrence Periods of Forced Novae
• Long-term evolution of surviving companion stars of Type Iax supernovae
• Rates and delay times of Type Ia supernovae in the helium-enriched main-sequence donor scenario
• White dwarf deflagrations for Type Iax supernovae: Polarisation signatures from the explosion and companion interaction
• SNe Ia as a cosmological probe
• Common envelope to explosion delay time distribution (CEEDTD) of type Ia supernovae
• Theoretical Delay Time Distributions
• Star formation history, double degenerates and type Ia supernovae in the thin disc
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• The envelope mass of red giant donors in Type Ia supernova progenitors
• Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
• The formation of type Ia supernovae from carbon-oxygen-silicon white dwarfs
• The radial distribution of supernovae compared to star formation tracers
• Ultraviolet studies of interacting binaries
• Off-centre carbon burning in He-accreting carbon-oxygen white dwarfs
• Hot subdwarf B stars with neutron star components II: Binary population synthesis
• The Gravitational Wave Emission of Double White Dwarf Coalescences
• A long-period pre-ELM system discovered from LAMOST medium-resolution survey
• Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?
• Constraining the Progenitor of the Type Ia Supernova SN 2012cg
• Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
• Evidence for bimodal orbital separations of white dwarf-red dwarf binary stars
• Binary population synthesis study on supersoft X-ray phase of single degenerate type Ia supernova progenitors
• Is the central binary system of the planetary nebula Henize 2-428 a Type Ia supernova progenitor?
• The Contribution of Chemical Abundances in Nova Ejecta to the Interstellar Medium
• On the White Dwarf Mass Problem of Cataclysmic Variables
• Type Ia Supernova Progenitor Properties and Their Host Galaxies
• The effect of metallicity on the delay-time distribution of type Ia supernova
• Can the Helium-Enriched Main-Sequence Donor Scenario Hide Enough Hydrogen to Explain Type Ia Supernovae?
• QU Carinae: a SNeIa progenitor?
• The two most recent thermonuclear supernovae in the Local Group: radio constraints on their progenitors and evolution
• Numerical Modelling of Tertiary Tides
• Shadows of our Former Companions: How the Single-Degenerate Binary Type Ia Supernova Scenario Affects Remnants
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• The effect of aspherical stellar wind of giant stars on the symbiotic channel of type Ia supernovae
• The correlation between C/O ratio, metallicity and the initial WD mass for SNe Ia
• Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
• WD + He star systems as the progenitors of Type Ia supernovae and their surviving companion stars
• Effects of Rotationally-Induced Mixing in Compact Binary Systems with Low-Mass Secondaries and in Single Solar-Type Stars
• The progenitors of Type Ia supernovae with asymptotic giant branch donors
• On the optical transients from double white-dwarf mergers
• Type Ia supernova ejecta-donor interaction: explosion model comparison
• Possible white dwarf progenitors of type Ia supernovae
• 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
• A closer look at non-interacting He stars as a channel for producing the old population of Type Ia supernovae
• White dwarf -- red giant star binaries as Type Ia supernova progenitors: with and without magnetic confinement
• A super-Eddington wind scenario for the progenitors of type Ia supernovae: binary population synthesis calculations
• The core degenerate scenario for the type Ia supernova SN 2020eyj
• Type Ia supernovae in the star formation deserts of spiral host galaxies
• Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors
• Dark Matter-Induced Baryonic Feedback in Galaxies
• Is SN 2006X from a WD + MS system with optically thick wind?
• WD+MS Systems as the Progenitors of Type Ia Supernovae with Different Metallicities
• The impact of binary star yields on the spectra of galaxies
• A Study of Magnetized White Dwarf + Helium Star Binary Evolution to Type Ia Supernovae
• Synthesis of radioactive elements in novae and supernovae and their use as a diagnostic tool
• A strange dwarf scenario for the formation of the peculiar double white dwarf binary SDSS J125733.63+542850.5
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• Three-dimensional simulations of accretion flow in the progenitor of Tycho's supernova
• Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
• Simplified Hydrostatic Carbon Burning in White Dwarf Interiors
• Non-LTE models for synthetic spectra of type Ia supernovae. III. An accelerated lambda iteration procedure for the mutual interaction of strong spectral lines in SN Ia models with and without energy deposition
• On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae
• Binary Evolutionary Models
• Type Ia Supernovae from First-generation Stars
• Modelling the chemical evolution of the Milky Way
• Pre-explosion helium shell flash in type Ia supernovae
• The cooling time of white dwarfs produced from type Ia supernovae
• Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
• Past and future of the central double-degenerate core of Henize 2-428
• Detecting milli-Hz gravitational waves with optical resonators
• Formation of millisecond pulsars with wide orbits
• Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb
• WD + MS systems as the progenitor of SNe Ia
• The timescales of chemical enrichment in the Galaxy
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss
• Double-detonation explosions as progenitors of type Iax supernovae
• SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart
• White Dwarf Mass Growth in Cataclysmic Variables: Roles of Dwarf Novae
• Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae
• Three-Dimensional Simulations of Type Ia Supernova Remnants I: Effects of a Main-Sequence Companion Star