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Titlebook: White Dwarfs: Cosmological and Galactic Probes; Edward M. Sion,Stéphane Vennes,Harry L. Shipman Book 2005 Springer Science+Business Media

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書(shū)目名稱White Dwarfs: Cosmological and Galactic Probes
編輯Edward M. Sion,Stéphane Vennes,Harry L. Shipman
視頻videohttp://file.papertrans.cn/1028/1027975/1027975.mp4
叢書(shū)名稱Astrophysics and Space Science Library
圖書(shū)封面Titlebook: White Dwarfs: Cosmological and Galactic Probes;  Edward M. Sion,Stéphane Vennes,Harry L. Shipman Book 2005 Springer Science+Business Media
描述.The emphasis on white dwarf stars and cosmology arises from the most recent advances in cosmological and galactic structure research in which white dwarf stars are playing a very prominent role.?Examples are?Type Ia supernovae (i.e. white dwarf supernovae), the origin and evolution of the universe, the age of the galactic disk, cosmochronology using white dwarfs in globular clusters and galactic clusters, and?the physics of accretion onto compact (very dense) stars. As an assisting guide to the reader, we have included, by invitation,?comprehensive review articles in each of the four major areas of the book, white dwarf supernovae, cosmology, accretion physics and galactic structure. The reviews include introductory material that they build upon...The book is suitable and most useful to advanced undergraduates, graduate students and scientific professionals (e.g. astronomers, astrophysicists, cosmologists, physicists). .
出版日期Book 2005
關(guān)鍵詞Bulge; Cosmology; Star; Type Ia supernovae; Universe; White dwarf stars; accretion physics; cosmochronology
版次1
doihttps://doi.org/10.1007/1-4020-3725-2
isbn_softcover978-90-481-6932-0
isbn_ebook978-1-4020-3725-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media B.V. 2005
The information of publication is updating

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Dark Halo Baryons not in Ancient White Dwarfs?mpact stellar objects in the dark mass is still poorly constrained. Microlensing experiments support the hypothesis that part of the Milky Way dark halo might be made of MACHOs with masses in the range 0.5– 0.8 solar mass. Ancient white dwarfs are generally considered as the most plausible candidate
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Study of the Galactic Bulge Using New Planetary Nebulae Discovered on the AAO/UKST Hα Surveylge. Such objects are excellent tracers for Bulge dynamical studies, are less affected by metallicity bias and have strong emission lines facilitating accurate velocities. We present preliminary results on plans to exploit these significant new Bulge PNe. Until now the relatively small numbers previ
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