Pre-Supernova Evolution of Massive Single and Binary Stars
arXiv:1206.5443 · doi:10.1146/annurev-astro-081811-125534
Abstract
Massive stars are essential to understand a variety of branches of astronomy including galaxy and star cluster evolution, nucleosynthesis and supernovae, pulsars and black holes. It has become evident that massive star evolution is very diverse, being sensitive to metallicity, binarity, rotation, and possibly magnetic fields. While the problem to obtain a good statistical observational database is alleviated by current large spectroscopic surveys, it remains a challenge to model these diverse paths of massive stars towards their violent end stage. We show that the main sequence stage offers the best opportunity to gauge the relevance of the various possible evolutionary scenarios. This also allows to sketch the post-main sequence evolution of massive stars, for which observations of Wolf-Rayet stars give essential clues. Recent supernova discoveries due to the current boost in transient searches allow tentative mappings of progenitor models with supernova types, including pair instability supernovae and gamma-ray bursts.
57 pages, 10 figures; free link to complete published paper: http://www.annualreviews.org/eprint/kf2CFBEBKi93fbcGJCBW/full/10.1146/annurev-astro-081811-125534
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- The Carnegie Supernova Project I: photometry data release of low-redshift stripped-envelope supernovae
- Population Synthesis of Isolated Neutron Stars with magneto-rotational evolution II: from radio-pulsars to magnetars
- The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
- The young massive SMC cluster NGC 330 seen by MUSE II. Multiplicity properties of the massive-star population
- The very young resolved stellar populations around stripped-envelope supernovae
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- The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
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- Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC
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- Aluminium-26 from massive binary stars I: non-rotating models
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- The deep OB star population in Carina from the VST Photometric H Survey (VPHAS+)
- Massive stars dying alone: The extremely remote environment of SN 2009ip
- Numerical experiments to help understand cause and effect in massive star evolution
- Non-interacting black hole binaries with Gaia and LAMOST
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- Massive stars in the Small Magellanic Cloud : Evolution, rotation and surface abundances
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- Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
- Spindown of massive main sequence stars in the Milky Way
- X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
- The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes
- The nature of the Cygnus extreme B-supergiant 2MASS J20395358+4222505
- Two circumstellar nebulae discovered with the Wide-field Infrared Survey Explorer and their massive central stars
- Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters
- Ultraviolet Spectropolarimetry with Polstar: Clumping and Mass-loss Rate Corrections
- Stellar evolution, SN explosion, and nucleosynthesis
- Two New Rapidly-Rotating ON Stars Found With LAMOST
- Thermodynamics of the Condensation of Dust Grains in Wolf-Rayet Stellar Winds
- The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material
- The VLT-FLAMES Tarantula Survey
- X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Putting the bi-stability jump to the test in the LMC
- Luminous, rapidly declining supernovae as stripped transitional objects in low metallicity environments: the case of SN 2022lxg
- Probing Massive Stars Around Gamma-Ray Burst Progenitors
- The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
- NGC 663 as a laboratory for massive star evolution
- Detailed Simulations of Massive Hierarchical Triple Star Systems - Exploring the impact of the stellar physics on the evolutionary pathways of massive hierarchical triple systems
- Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
- Probing the models: Abundances for high-mass stars in binaries
- Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
- Magnetic Fields in Stars: Origin and Impact
- Luminous Fast Blue Optical Transients as "Failed" Gravitational-wave Sources: Helium CoreBlack Hole Mergers Following Delayed Dynamical Instability
- The NGC 346 massive star census: Nitrogen abundances for apparently single, narrow lined, hydrogen core burning B-type stars
- Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
- SiO maser polarization and magnetic field in evolved cool stars
- Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
- Towards Multi Energy Neutrino Astronomy: Diagnosing Enhanced Circumstellar Material around Stripped-Envelope Supernovae
- The rich molecular environment of the luminous blue variable star AFGL 2298
- A near-UV reconnaissance of metal-poor massive stars
- MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations
- Four open questions in massive star evolution
- Fundamental parameters of the massive eclipsing binary HM1 8
- Rotational Dynamics in Pulsational Pair-Instability Supernovae: Implications for Mass-Loss and Transient Events
- Observed Consequences of Presupernova Instability in Very Massive Stars
- Pulsation and Mass Loss Across the HR Diagram: From OB stars to Cepheids to Red Supergiants
- Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions
- Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star Zeta Oph from high-cadence ESPRESSO spectroscopy and TESS photometry
- Formation of massive close binaries I. Detached evolution
- Rotational velocities of single and binary O-type stars in the Tarantula Nebula
- Discovery of an optical cocoon tail behind the runaway HD 185806
- JWST Detection of Hydrocarbon Ices and Methane Gas on Makemake
- Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
- A stringent upper limit on Be star fractions produced by binary interaction
- Bridging the Gap: From Massive Stars to Supernovae
- Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
- High resolution observations of Cen A: Yellow and red supergiants in a region of jet-induced star formation?
- Constraining the progenitor evolution of GW 150914
- Interacting supernovae and where to find them
- Modelling binary rotating stars by new population synthesis code BONNFIRES
- Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
- Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
- High-mass stars in Milky Way clusters
- FLUID: A rocket-borne pathfinder instrument for high efficiency UV band selection imaging
- Asteroseismology
- A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
- Massive stars in the Tarantula Nebula: A Rosetta Stone for Extragalactic Supergiant HII Regions
- Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images
- Electron-capture Supernova Candidates from Light Curves: Implications for Their Progenitors and Explosion Properties
- Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins
- Estimating Transient Rates from Cosmological Simulations and BPASS
- Discovery of O stars in the tidal Magellanic Bridge: Stellar parameters, abundances, and feedback of the nearest metal-poor massive stars and their implication for the Magellanic System ecology
- Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad
- Oxygen and silicon abundances in Cygnus OB2: Chemical homogeneity in a sample of OB slow rotators
- Accretion in massive colliding wind binaries and the effect of wind momentum ratio
- Non-parametric identification of single-lined binary candidates in young clusters using single-epoch spectroscopy
- Progenitors of Core-Collapse Supernovae
- Constraining Black Hole Natal Kicks with Astrometric Microlensing
- Radio Spectral Energy Distributions for Single Massive Star Winds with Free-Free and Synchrotron Emission
- Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
- Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning
- Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey
- Massive stars evolution: feedbacks in low-Z environment
- New mass estimates for massive binary systems: a probabilistic approach using polarimetric radiative transfer
- Two Nested Shells around the Blue Supergiant ALS 19653
- The OVz stars in NGC 346: distribution, stellar parameters and insights into low-metallicity effects
- Expectation for the MeV Gamma-Ray Emission from Pair-Instability Supernovae
- Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
- A database of spectral energy distributions of progenitors of core-collapse supernovae
- One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations
- Formation of black holes from He stars
- Chemical fingerprints of binary mass transfer in massive stars
- The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry