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Titlebook: Gas Accretion onto Galaxies; Andrew Fox,Romeel Davé Book 2017 Springer International Publishing AG 2017 Accretion in Galaxies.Accretion Mo

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發(fā)表于 2025-3-21 19:53:16 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Gas Accretion onto Galaxies
編輯Andrew Fox,Romeel Davé
視頻videohttp://file.papertrans.cn/381/380724/380724.mp4
概述Includes contributions from leading accretion experts on both observational data and on computer models.Elaborates on the baryon cycle, one of the central questions in the 2010 Astronomy Decadal Surve
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Gas Accretion onto Galaxies;  Andrew Fox,Romeel Davé Book 2017 Springer International Publishing AG 2017 Accretion in Galaxies.Accretion Mo
描述.This edited volume presents the current state of gas accretion studies from both observational and theoretical perspectives, and charts our progress towards answering the fundamental yet elusive question of how galaxies get their gas. Understanding how galaxies form and evolve has been a central focus in astronomy for over a century. These studies have accelerated in the new millennium, driven by two key advances: the establishment of a firm concordance cosmological model that provides the backbone on which galaxies form and grow, and the recognition that galaxies grow not in isolation but within a “cosmic ecosystem” that includes the vast reservoir of gas filling intergalactic space. This latter aspect in which galaxies continually exchange matter with the intergalactic medium via inflows and outflows has been dubbed the “baryon cycle”. The topic of this book is directly related to the baryon cycle, in particular its least well constrained aspect, namely gas accretion...Accretion is a rare area of astrophysics in which the basic theoretical predictions are established, but the observations have been as yet unable to verify the expectations. Accretion has long been seen around the
出版日期Book 2017
關(guān)鍵詞Accretion in Galaxies; Accretion Models in Astrophysics; Galactic Scale Accretion; Gas Behavior in Gala
版次1
doihttps://doi.org/10.1007/978-3-319-52512-9
isbn_softcover978-3-319-84920-1
isbn_ebook978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing AG 2017
The information of publication is updating

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發(fā)表于 2025-3-21 21:40:07 | 只看該作者
0067-0057 of the central questions in the 2010 Astronomy Decadal Surve.This edited volume presents the current state of gas accretion studies from both observational and theoretical perspectives, and charts our progress towards answering the fundamental yet elusive question of how galaxies get their gas. Unde
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Multiregional Projection and Stable Growth,he most recent studies follows that the present-day gas accretion rate of the Milky Way is a few solar masses per year, which is sufficient to maintain the Galaxy’s star-formation rate at its current level.
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Gas Accretion onto the Milky Way,he most recent studies follows that the present-day gas accretion rate of the Milky Way is a few solar masses per year, which is sufficient to maintain the Galaxy’s star-formation rate at its current level.
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The Effect of Galactic Feedback on Gas Accretion and Wind Recycling,s than gas accreting for the first time. Quantitative conclusions, however, vary between studies, because the amount of wind recycling is dependent on the details of the feedback model. We discuss these differences, known caveats, and ways to make progress in understanding how galaxies are fed at low redshift.
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