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Titlebook: Galactic Bulges; Eija Laurikainen,Reynier Peletier,Dimitri Gadotti Book 2016 Springer International Publishing Switzerland 2016 Dark Matte

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發(fā)表于 2025-3-21 16:15:27 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Galactic Bulges
編輯Eija Laurikainen,Reynier Peletier,Dimitri Gadotti
視頻videohttp://file.papertrans.cn/381/380330/380330.mp4
概述Addresses the key open question - what is the fraction of galaxies with no classical bulges in the local Universe.Attempts to clarify the role of the various types of bulges during the mass build-up o
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Galactic Bulges;  Eija Laurikainen,Reynier Peletier,Dimitri Gadotti Book 2016 Springer International Publishing Switzerland 2016 Dark Matte
描述This book consists of invited reviews on Galactic Bulges written by experts in the field. A central point of the book is that, while in the standard picture of galaxy formation a significant amount of the baryonic mass is expected to reside in classical bulges, the question what is the fraction of galaxies with no classical bulges in the local Universe has remained open. The most spectacular example of a galaxy with no significant classical bulge is the Milky Way. The reviews of this book attempt to clarify the role of the various types of bulges during the mass build-up of galaxies, based on morphology, kinematics and stellar populations and connecting their properties at low and high redshifts. The observed properties are compared with the predictions of the theoretical models, accounting for the many physical processes leading to the central mass concentration and their destruction in galaxies. This book serves as an entry point for PhD students and non-specialists and as a reference work for researchers in the field.
出版日期Book 2016
關鍵詞Dark Matter; Formation of Galactic Bulges; Galactic Bulges; Galaxy Formation and Evolution; Milky Way Bu
版次1
doihttps://doi.org/10.1007/978-3-319-19378-6
isbn_softcover978-3-319-37210-5
isbn_ebook978-3-319-19378-6Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer International Publishing Switzerland 2016
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A Universal Kinematic Scaling Relation and Galaxy Bulgesused fundamental plane in certain contexts. We then examine whether bulges separately satisfy the FM relation and discuss what the success or failure of such a match implies for the nature of classical- and pseudo-bulges. On the basis of this preliminary analysis we suggest that while classical bulg
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Theoretical Models of the Galactic Bulge witnessed a gradual paradigm shift in the formation and evolution of the Galactic bulge. Bulges were commonly believed to form in the dynamical violence of galaxy mergers. However, it has become increasingly clear that the main body of the Milky Way bulge is not a classical bulge made by previous m
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Galaxy Bulges and Their Massive Black Holes: A Reviewnce of massive black holes at the centers of galaxies. It then presents the historical development of the near-linear (black hole)–(host spheroid) mass relation, before explaining why this has recently been dramatically revised. Past disagreement over the slope of the (black hole)–(velocity dispersi
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