Rates and delay times of Type Ia supernovae in the helium-enriched main-sequence donor scenario
arXiv:1801.05810 · doi:10.1093/mnras/sty172
Abstract
The nature of the progenitors of Type Ia supernovae (SNe Ia) remains a mystery. Comparing theoretical rates and delay-time distributions of SNe Ia with those inferred observationally can constrain their progenitor models. In this work, taking thermohaline mixing into account in the helium-enriched main-sequence (HEMS) donor scenario, we address rates and delay times of SNe Ia in this channel by combining the results of self-consistent binary evolution calculations with population synthesis models. We find that the Galactic SN Ia rate from the HEMS donor scenario is around 0.6-1.2 per century, which is about 30% of the observed rate. Delay times of SNe Ia in this scenario cover a wide range of 0.1-1.0 Gyr. We also present the pre-explosion properties of companion stars in the HEMS donor scenario, which will be helpful for placing constraints on SN Ia progenitors through analyzing their pre-explosion images.
arXiv comment11 pages, 8 figures, Accepted for publication in MNRAS
References in corpus (120)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Evolution of binary stars and the effect of tides on binary populations
- Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
- Type Ia Supernova Explosion Models
- Observational clues to the progenitors of Type-Ia supernovae
- Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample
- The Origin of Subdwarf B Star (I): the Formation Channels
- Approximate input physics for stellar modelling
- Nearby Supernova Rates from the Lick Observatory Supernova Search. III. The Rate-Size Relation, and the Rates as a Function of Galaxy Hubble Type and Colour
- Normal Type Ia supernovae from violent mergers of white dwarf binaries
- Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?
- The single degenerate channel for the progenitors of type Ia supernovae
- Seeing the Collision of a Supernova with its Companion Star
- Faint Thermonuclear Supernovae from AM Canum Venaticorum Binaries
- Population synthesis for double white dwarfs I.Close detached systems
- Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with M~0.9 M_sun
- Type Iax Supernovae: A New Class of Stellar Explosion
- Detonations in Sub-Chandrasekhar Mass C+O White Dwarfs
- A Wide Symbiotic Channel to Type Ia Supernovae
- Detection of circumstellar material in a normal Type Ia Supernova
- Progenitors of type Ia supernovae
- Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and its Consequences
- PTF11kx: A Type-Ia Supernova with a Symbiotic Nova Progenitor
- Toward a Unification of Star Formation Rate Determinations in the Milky Way and Other Galaxies
- Rates and Delay Times of Type Ia Supernovae
- Sub-Chandrasekhar Mass Models For Type Ia Supernovae
- Constraints on the Progenitor System of the Type Ia Supernova SN 2011fe/PTF11kly
- Accelerating Compact Object Mergers in Triple Systems with the Kozai Resonance: A Mechanism for "Prompt" Type Ia Supernovae, Gamma-Ray Bursts, and Other Exotica
- A Compact Degenerate Primary-Star Progenitor of SN 2011fe
- The delay-time distribution of type-Ia supernovae from Sloan II
- Double-detonation sub-Chandrasekhar supernovae: synthetic observables for minimum helium shell mass models
- A Circumbinary Disk in the Final Stages of Common Envelope and the Core-Degenerate Scenario for Type Ia Supernovae
- The binary progenitor of Tycho Brahe's 1572 supernova
- Head-on collisions of white dwarfs in triple systems could explain type Ia supernova
- Theoretical uncertainties of the type Ia supernova rate
- Formation of contact in massive close binaries
- Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features
- Type Ia Supernovae Strongly Interacting with Their Circumstellar Medium
- Surface Detonations in Double Degenerate Binary Systems Triggered by Accretion Stream Instabilities
- SN 2008ha: An Extremely Low Luminosity and Extremely Low Energy Supernova
- Violent mergers of nearly equal-mass white dwarf as progenitors of subluminous Type Ia supernovae
- The supernova delay time distribution in galaxy clusters and implications for Type-Ia progenitors and metal enrichment
- Constraining the Type Ia Supernova Progenitor: The Search for Hydrogen in Nebular Spectra
- Strong Ultraviolet Pulse From a Newborn Type Ia Supernova
- Collisions of white dwarfs as a new progenitor channel for type Ia supernovae
- Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and Observables
- Evolution of the Milky Way with radial motions of stars and gas I. The solar neighborhood and the thin and thick disk
- Star formation, supernovae, iron, and alpha: consistent cosmic and Galactic histories
- EVLA Observations Constrain the Environment and Progenitor System of Type Ia Supernova 2011fe
- A three-dimensional deflagration model for Type Ia supernovae confronted with observations
- Type-Ia Supernova Rates to Redshift 2.4 from CLASH: the Cluster Lensing And Supernova survey with Hubble
- Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?
- A luminous, blue progenitor system for a type-Iax supernova
- Low and intermediate-mass close binary evolution and the initial - final mass relation
- Nearby Supernova Rates from the Lick Observatory Supernova Search. IV. A Recovery Method for the Delay Time Distribution
- SN~2012cg: Evidence for Interaction Between a Normal Type Ia Supernova and a Non-Degenerate Binary Companion
- Have the Elusive Progenitors of Supernovae Type Ia Been Discovered?
- Delay Times and Rates for Type Ia Supernovae and Thermonuclear Explosions from Double-detonation Sub-Chandrasekhar Mass Models
- Modelling the binary progenitor of supernova 1993J
- The Initiation and Propagation of Helium Detonations in White Dwarf Envelopes
- Supernova rates from the Southern inTermediate Redshift ESO Supernova Search (STRESS)
- Three-Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae
- Early Blue Excess from the Type Ia Supernova 2017cbv and Implications for Its Progenitor
- Impact of type ia supernova ejecta on binary companions in the single-degenerate scenario
- On Type Ia Supernovae From The Collisions of Two White Dwarfs
- Early radio and X-ray observations of the youngest nearby type Ia supernova PTF11kly (SN 2011fe)
- Subaru high-resolution spectroscopy of Star G in the Tycho supernova remnant
- Deflagrations in hybrid CONe white dwarfs: a route to explain the faint Type Iax supernova 2008ha
- Type Ia Supernovae: An Examination of Potential Progenitors and the Redshift Distribution
- No X-rays from the very nearby Type Ia SN2014J: constraints on its environment
- Discovery of 90 Type Ia supernovae among 700,000 Sloan spectra: the Type-Ia supernova rate versus galaxy mass and star-formation rate at redshift ~0.1
- He-Accreting WDs: accretion regimes and final outcomes
- Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
- The delay time distribution of type Ia supernovae: a comparison between theory and observation
- Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
- The progenitors of Type Ia supernovae with long delay times
- How the merger of two white dwarfs depends on their mass ratio: orbital stability and detonations at contact
- Type IA supernovae from very long delayed explosion of core - WD merger
- The supernova rate in local galaxy clusters
- PopCORN: Hunting down the differences between binary population synthesis codes
- An unusual white dwarf star may be a surviving remnant of a subluminous Type Ia supernova
- Constraints on the Progenitor System of the Type Ia Supernova 2014J from Pre-Explosion Hubble Space Telescope Imaging
- Early light curves for Type Ia supernova explosion models
- 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
- A New Estimation of Mass Accumulation Efficiency in Helium Shell Flashes toward Type Ia Supernova Explosions
- A reconnaissance of the possible donor stars to the Kepler supernova
- Searching for swept-up Hydrogen and Helium in the late-time spectra of 11 nearby Type Ia supernovae
- Slow-Speed Supernovae from the Palomar Transient Factory: Two Channels
- The effect of helium accretion efficiency on rates of Type Ia supernovae: double-detonations in accreting binaries
- The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?
- Hydrogen and helium in the spectra of Type Ia supernovae
- Environment-derived constraints on the progenitors of low-luminosity type I supernovae
- Strong Evidence Against A Non-Degenerate Companion in SN 2012cg
- A High-Resolution Spectroscopic Search for the Remaining Donor for Tycho's Supernova
- Companion Stars of Type Ia Supernovae
- The effects of thermohaline mixing on low-metallicity asymptotic giant branch stars
- Evolution Of Post-Impact Remnant Helium Stars In Type Ia Supernova Remnants Within The Single-Degenerate Scenario
- Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T
- A comprehensive progenitor model for SNe Ia
- Beyond the bubble catastrophe of Type Ia supernovae: Pulsating Reverse Detonation models
- The Detonation Mechanism of the Pulsationally-Assisted Gravitationally-Confined Detonation Model of Type Ia Supernovae
- Single degenerate supernova type Ia progenitors
- A common-envelope wind model for Type Ia supernovae (I): binary evolution and birth rate
- He II recombination lines as a test of the nature of SN Ia progenitors in elliptical galaxies
- Progenitor constraints on the Type-Ia supernova SN2011fe from pre-explosion Hubble Space Telescope HeII narrow-band observations
- Pulsating reverse detonation models of Type Ia supernovae. I: Detonation ignition
- A Search for a Surviving White Dwarf Companion in SN 1006
- Improved Hubble Space Telescope Proper Motions for Tycho-G and Other Stars in the Remnant of Tycho's Supernova 1572
- The rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario
- Constraints on single-degenerate Chandrasekhar mass progenitors of Type Iax supernovae
- Diffuse Gas in Galaxies Sheds New Light on the Origin of Type Ia Supernovae
- Smoothed Particle Hydrodynamics simulations of the core-degenerate scenario for Type Ia supernovae
- Pre-explosion companion stars in Type Iax supernovae
- Early ultraviolet signatures from the interaction of Type Ia supernova ejecta with a stellar companion
- The Evolution of the Type Ia Supernova Luminosity Function
- Early UV emission from disk-originated matter (DOM) in type Ia supernovae in the double degenerate scenario
- Constraining the Progenitor of the Type Ia Supernova SN 2012cg
- Can the Helium-Enriched Main-Sequence Donor Scenario Hide Enough Hydrogen to Explain Type Ia Supernovae?
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- Type Ia Supernova Explosions in Binary Systems: A Review
- The Physics of Star Cluster Formation and Evolution
- Supernovae Ia in 2019 (review): a rising demand for spherical explosions
- Binary Stars in the New Millennium
- Long-term evolution of surviving companion stars of Type Iax supernovae
- Signatures of a surviving helium-star companion in Type Ia supernovae and constraints on the progenitor companion of SN 2011fe
- Type Ia supernova ejecta-donor interaction: explosion model comparison
- 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
- A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
- Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
- On the rotation properties of a post-explosion helium-star companion in Type Iax supernovae