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Related papers: Binary Fraction Indicators in Resolved Stellar Pop…

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We compare our latest single and binary stellar model results from the Cambridge STARS code to several sets of observations. We examine four stellar population ratios, the number of blue to red supergiants, the number of Wolf-Rayet stars to…

Astrophysics · Physics 2009-11-13 John J. Eldridge , Robert G. Izzard , Christopher A. Tout

Populations of massive stars are directly reflective of the physics of stellar evolution. Counting subtypes of massive stars and ratios of massive stars in different evolutionary states have been used ubiquitously as diagnostics of age and…

Solar and Stellar Astrophysics · Physics 2018-11-14 Trevor Z. Dorn-Wallenstein , Emily M. Levesque

We present our models of the effect of binaries on high-resolution spectroscopic surveys. We want to determine how many binary stars will be observed, whether unresolved binaries will contaminate measurements of chemical abundances, and how…

Solar and Stellar Astrophysics · Physics 2018-08-22 Edita Stonkute , Ross P. Church , Sofia Feltzing , Jennifer A. Johnson

Binary stars are important for a full understanding of stellar evolution. We present a summary of how predictions of the relative supernova rates varies between single and binary stars. We also show how the parameter space of different…

Astrophysics · Physics 2007-05-23 J. J. Eldridge

Binary population synthesis is the method by which predictions of varied observables of stellar populations can be made from theoretical models of binary stellar evolution. Binary stars have many more possible evolutionary outcomes compared…

Solar and Stellar Astrophysics · Physics 2020-06-15 J. J. Eldridge

How massive stars end their lives depends on the core mass, core angular momentum, and hydrogen envelopes at death. However, these key physical facets of stellar evolution can be severely affected by binary interactions. In turn, the…

High Energy Astrophysical Phenomena · Physics 2023-11-27 Tomoya Kinugawa , Shunsaku Horiuchi , Tomoya Takiwaki , Kei Kotake

Binary stars have been shown to have a substantial impact on the integrated light of stellar populations, particularly at low metallicity and early ages - conditions prevalent in the distant Universe. But the fraction of stars in stellar…

Astrophysics of Galaxies · Physics 2020-05-06 E. R. Stanway , A. A. Chrimes , J. J. Eldridge , H. F. Stevance , .

The effects of binaries on population studies of stars and stellar phenomena have been investigated over the past 3 decades by many research groups. Here we will focus mainly on the work that has been done recently in Brussels and we will…

Astrophysics · Physics 2009-11-10 D. Vanbeveren

Wolf-Rayet stars (WRs) represent the end of a massive star's life as it is about to turn into a supernova. Obtaining complete samples of such stars across a large range of metallicities poses observational challenges, but presents us with…

Solar and Stellar Astrophysics · Physics 2019-08-20 Kathryn F. Neugent , Philip Massey

Knowledge of the binary population in stellar groupings provides important information about the outcome of the star forming process in different environments (see, e.g., Blaauw 1991, and references therein). Binarity is also a key…

Binaries are very common in galaxies, and more than half of Galactic hot subdwarf stars, which are thought as a possible origin of UV-upturn of old stellar populations, are found in binaries. Previous works showed that binary evolution can…

Astrophysics of Galaxies · Physics 2015-06-12 Zhongmu Li , Caiyan Mao , Li Chen , Qian Zhang , Maocai Li

Knowledge of the binary population in stellar groupings provides important information about the outcome of the star forming process in different environments. Binarity is also a key ingredient in stellar population studies and is a…

The evolution of massive stars in general, massive close binaries in particular depend on processes where, despite many efforts, the physics are still uncertain. Here we discuss the effects of stellar wind as function of metallicity during…

Astrophysics · Physics 2007-05-23 D. Vanbeveren

Many aspects of the evolution of stars, and in particular the evolution of binary stars, remain beyond our ability to model them in detail. Instead, we rely on observations to guide our often phenomenological models and pin down uncertain…

Solar and Stellar Astrophysics · Physics 2018-08-22 Robert G. Izzard , Ghina M. Halabi

Our uncertainties about binary star systems (and triples and so on) limit our capabilities in literally every single one of the Thematic Areas identified for Astro2020. We need to understand the population statistics of stellar multiplicity…

We have constructed a new code to produce synthetic spectra of stellar populations that includes massive binaries. We have tested this code against the broadband colours of unresolved young massive stellar clusters in nearby galaxies, the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 John J. Eldridge , Elizabeth R. Stanway

Stellar systems composed of single, double, triple or high-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through…

Using our new Binary Population and Spectral Synthesis (BPASS) code we explore the affect of binary populations on the integrated spectra of galaxies. We also explore the interplay of binary populations and a varying maximum stellar mass.…

Solar and Stellar Astrophysics · Physics 2010-08-10 John J Eldridge

Binary stars plays important role in the evolution of stellar populations . The intrinsic binary fraction ($f_{bin}$) of O and B-type (OB) stars in LAMOST DR5 was investigated in this work. We employed a cross-correlation approach to…

Solar and Stellar Astrophysics · Physics 2022-01-05 Feng Luo , Yong-Heng Zhao , Jiao Li , Yan-Jun Guo , Chao Liu

Massive stars are born predominantly as members of binary (or higher multiplicity) systems, and the presence of a companion can significantly alter their life and final fate. Therefore, any observed sample of massive stars or associated…

Solar and Stellar Astrophysics · Physics 2020-04-14 Mathieu Renzo , Emmanouil Zapartas
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