The influence of binaries on galactic chemical evolution
arXiv:astro-ph/0410024 · doi:10.1016/j.newar.2004.07.001
Abstract
Understanding the galaxy in which we live is one of the great intellectual challenges facing modern science. With the advent of high quality observational data, the chemical evolution modeling of our galaxy has been the subject of numerous studies in the last years. However, all these studies have one missing element which is the evolution of close binaries. Reason: their evolution is very complex and single stars only perhaps can do the job. (Un)Fortunately at present we know that the majority of the observed stars are members of a binary or multiple system and that certain objects can only be formed through binary evolution. Therefore galactic studies that do not account for close binary evolution may be far from realistic. Because of the large expertise developed through the years in stellar evolution in general and binary evolution in particular at the Brussels Astrophysical Institute, we found ourselves in a privileged position to be the first to do chemical evolutionary simulations with the inclusion of detailed binary evolution. The complexity of close binary evolution has kept many astronomers from including binary stars into their studies. However, it is not always the easiest way of living that gives you the most excitement and satisfaction.
115 pages, many figures and tables
References in corpus (72)
- The Global Schmidt Law in Star Forming Galaxies
- Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
- Discovery of the peculiar supernova 1998bw in the error box of GRB980425
- The Geneva-Copenhagen survey of the Solar neighbourhood: Ages, metallicities, and kinematic properties of 14,000 F and G dwarfs
- Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
- A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
- The Chemical Evolution of the Galaxy: the two-infall model
- Galactic Chemical Evolution: Hydrogen Through Zinc
- Abundance Gradients and the Formation of the Milky Way
- Neutron Star Mass Measurements. I. Radio Pulsars
- The Velocity Distribution of Isolated Radio Pulsars
- Stellar evolution with rotation VIII: Models at Z = 10^{-5} and CNO yields for early galactic evolution
- Mass Limits For Black Hole Formation
- Neutron-Capture Elements in the Early Galaxy: Insights from a Large Sample of Metal-Poor Giants
- The unusual afterglow of GRB 980326: evidence for the gamma-ray burst/supernova connection
- Formation Rates of Black Hole Accretion Disk Gamma-Ray Bursts
- Chemical yields from low- and intermediate-mass stars: model predictions and basic observational constraints
- The Pulsar Kick Velocity Distribution
- The Maximum Mass of a Neutron Star
- A Wide Symbiotic Channel to Type Ia Supernovae
- Chemo-spectrophotometric evolution of spiral galaxies: I. The model and the Milky Way
- Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy
- Jet-Induced Explosions of Core Collapse Supernovae
- On the typical timescale for the chemical enrichment from SNeIa in Galaxies
- Core-Collapse Simulations of Rotating Stars
- Galactic chemical evolution of heavy elements: from Barium to Europium
- Low-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution
- Nucleosynthesis in Type II Supernovae
- Galaxy Formation: CDM, Feedback and the Hubble Sequence
- Composition, Structure and Evolution of Neutron Stars with Kaon Condensates
- A Black Hole in the Superluminal source SAX J1819.3-2525 (V4641 Sgr)
- Oxygen abundances in unevolved metal-poor stars from near-UV OH lines
- O/Fe in metal-poor main sequence and subgiant stars
- On the galactic disc age-metallicity relation
- The r-Process in Neutrino-Driven Winds from Nascent, "Compact" Neutron Stars of Core-Collapse Supernovae
- Massive Stars in the Range : Evolution and Nucleosynthesis. II. the Solar Metallicity Models
- Chemistry and Kinematics in the Solar Neighborhood: Implications for Stellar Populations and for Galaxy Evolution
- Inward Propagation of Nuclear-Burning Shells in Merging C-O and He White Dwarfs
- Chemo-spectrophotometric evolution of spiral galaxies: III. Abundance and colour gradients in discs
- Formation and coalescence of relativistic binary stars: effect of kick velocity
- Neutron Star Population Dynamics.I: Millisecond Pulsars
- The solar neighbourhood age-metallicity relation - does it exist?
- The History of the Comic Supernova Rate Derived from the Evolution of the Host Galaxies
- Abundances of Deuterium, Oxygen, and Nitrogen in the Local Interstellar Medium: Overview of First Results from the Far Ultraviolet Spectroscopic Explorer Mission
- The metallicity distribution of G dwarfs in the solar neighbourhood
- Explosive Nucleosynthesis in Hypernovae
- The evolution of naked helium stars with a neutron-star companion in close binary systems
- Enrichment of the r-process Element Europium in the Galactic Halo
- Intermediate mass stars: updated models
- The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems
- Complete and Simultaneous Spectral Observations of the Black-Hole X-ray Nova XTE J1118+480
- Star formation and chemical evolution in SPH simulations: a statistical approach
- Quantitative analysis of WC stars: Constraints on neon abundances from ISO/SWS spectroscopy
- Double Neutron Star Systems and Natal Neutron Star Kicks
- The Outer Regions of the Galactic Bulge:II Analysis
- Does low surface brightness mean low surface density?
- The Halo Black-Hole X-ray Transient XTE J1118+480
- HIPPARCOS age-metallicity relation of the solar neighbourhood disc stars
- The Earliest Phases of Galaxy Evolution
- Is High Primordial Deuterium Consistent With Galactic Evolution?
- Stellar Yields and Chemical Evolution I: Abundance Ratios and Delayed Mixing in the Solar Neighbourhood
- Implications of O and Mg abundances in metal-poor halo stars for stellar iron yields
- Chemical abundances and winds of massive stars in M31: a B-type supergiant and a WC star in OB10
- Inhomogeneous Chemical Evolution of the Galactic Halo: Abundance of r-process Elements
- The Chemical Evolution of the Galaxy with Variable IMFs
- Optical and Near Infrared Observations of the Afterglow of GRB 980329 from 15 Hours to 10 Days
- Parity Violation in Neutrino Transport and the Origin of Pulsar Kicks
- The galactic evolution of the supernova rates
- Near-Infrared Light Curves of the Black Hole Binary A0620-00
- Chemical evolution models with a new stellar nucleosynthesis
- The Chemical Evolution of the Solar Neighbourhood: the Effect of Binaries
- The chemical evolution of the Galaxy: the importance of stars with an initial mass larger than 40Mo
Cited by in corpus (53)
- Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
- Observational clues to the progenitors of Type-Ia supernovae
- Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
- The effect of massive binaries on stellar populations and supernova progenitors
- The Evolution of Compact Binary Star Systems
- Double Compact Objects III: Gravitational Wave Detection Rates
- COSMIC Variance in Binary Population Synthesis
- The impact of companions on stellar evolution
- Massive double compact object mergers: gravitational wave sources and r-process-element production sites
- eLISA eccentricity measurements as tracers of binary black hole formation
- Delay Times and Rates for Type Ia Supernovae and Thermonuclear Explosions from Double-detonation Sub-Chandrasekhar Mass Models
- The Effect of Different Type Ia Supernova Progenitors on Galactic Chemical Evolution
- Binary Population Synthesis
- The delay time distribution of type Ia supernovae: a comparison between theory and observation
- Towards a Realistic Explosion Landscape for Binary Population Synthesis
- Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
- Neutron Star Mergers as the Origin of r-Process Elements in the Galactic Halo Based on the Sub-halo Clustering Scenario
- PopCORN: Hunting down the differences between binary population synthesis codes
- The r-process in the neutrino-driven wind from a black-hole torus
- Can neutron star mergers alone explain the r-process enrichment of the Milky Way?
- Common-Envelope Episodes that lead to Double Neutron Star formation
- Multiple Stellar Evolution: a population synthesis algorithm to model the stellar, binary, and dynamical evolution of multiple-star systems
- The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
- On Rejuvenation in Massive Binary Systems
- Reexamining the temperature and neutron density conditions for r-process nucleosynthesis with augmented nuclear mass models
- The evolution of CNO elements in galaxies
- Population synthesis in astrophysics
- Nucleosynthesis of binary-stripped stars
- Stochastic Chemical Evolution of Galactic Subhalos and the Origin of r-Process Elements
- The delayed time distribution of massive double compact star mergers
- Blue supergiant progenitor models of Type II supernovae
- Towards a volumetric census of close white dwarf binaries I.Reference samples
- Neutron star mergers as the astrophysical site of the r-process in the Milky Way and its satellite galaxies
- The cosmic carbon footprint of massive stars stripped in binary systems
- Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
- Evidence from high mass X-ray binaries that Galactic WR components of WR+O binaries end their life with a supernova explosion
- Highly r-process enhanced stars in ultra-faint dwarf galaxies
- The effect of intermediate mass close binaries on the chemical evolution of Globular Clusters
- The evolution of massive and very massive stars in clusters
- Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074
- Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
- A comparison between observed Algol-type double stars in the Solar neighborhood and evolutionary computations of galactic case A binaries with a B-type primary at birth
- The impact of binary star yields on the spectra of galaxies
- Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
- Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
- Globular cluster formation with multiple stellar populations: A single-binary composite scenario
- Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
- The impact of rare events on the chemical enrichment in dwarf galaxies
- Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
- Binary populations and stellar dynamics in young clusters
- Modelling the chemical evolution
- Close Pairs as Probes of the Galaxy's Chemical Evolution
- Two distributions shedding light on supernova Ia progenitors: delay times and G-dwarf metallicities