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Titlebook: Ecology of Blue Straggler Stars; Henri M. J. Boffin,Giovanni Carraro,Giacomo Beccar Book 2015 Springer-Verlag Berlin Heidelberg 2015 Blue

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书目名称Ecology of Blue Straggler Stars
编辑Henri M. J. Boffin,Giovanni Carraro,Giacomo Beccar
视频video
概述Presents all the relevant aspects of blue straggler stars research including recent observations and theoretical models.Carefully edited extended contributions by well-known experts in blue straggler
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Ecology of Blue Straggler Stars;  Henri M. J. Boffin,Giovanni Carraro,Giacomo Beccar Book 2015 Springer-Verlag Berlin Heidelberg 2015 Blue
描述.The existence of blue straggler stars, which appear younger, hotter, and more massive than their siblings, is at odds with a simple picture of stellar evolution. Such stars should have exhausted their nuclear fuel and evolved long ago to become cooling white dwarfs. They are found to exist in globular clusters, open clusters, dwarf spheroidal galaxies of the Local Group, OB associations and as field stars..This book summarises the many advances in observational and theoretical work dedicated to blue straggler stars. Carefully edited extended contributions by well-known experts in the field cover all the relevant aspects of blue straggler stars research: Observations of blue straggler stars in their various environments; Binary stars and formation channels; Dynamics of globular clusters; Interpretation of observational data and comparison with models. The book also offers an introductory chapter on stellar evolution written by the editors of the book..
出版日期Book 2015
关键词Blue Straggler Formation; Blue Straggler Stars Overview; Dwarf Galaxies Stellar Population; Dynamical E
版次1
doihttps://doi.org/10.1007/978-3-662-44434-4
isbn_softcover978-3-662-51274-6
isbn_ebook978-3-662-44434-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer-Verlag Berlin Heidelberg 2015
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https://doi.org/10.1007/978-3-319-57228-4nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.
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Elementary Probability and Set Theory,y nebulae (CSPN). The most recent observations of cool CSPN progenitors of barium stars, as well as of carbon-rich post-common envelope systems, are providing unique constraints on the mass transfer processes.
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Wave Power and the Djursland Coast,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).
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Introduction to the Theory of Stellar Evolution,nitial mass. In this introductory chapter, we briefly review the most important aspects concerning the evolution and nucleosynthesis of single stars, form the early stage of its formation to the final stages and death.
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Formation Channels for Blue Straggler Stars,ing a primary close to the current turn-off mass. Rather, their primaries tend to be somewhat more massive and have evolved off the main sequence, filling their Roche lobes in the past, often converting their secondaries into blue straggler stars (but more than 1 Gyr or so ago and thus they are no longer visible today as blue straggler stars).
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