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Titlebook: New Light on Dark Stars; Red Dwarfs, Low-Mass I. Neill Reid,Suzanne L. Hawley Book 2005Latest edition Springer-Verlag Berlin Heidelberg 200

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發(fā)表于 2025-3-21 18:37:27 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱New Light on Dark Stars
副標(biāo)題Red Dwarfs, Low-Mass
編輯I. Neill Reid,Suzanne L. Hawley
視頻videohttp://file.papertrans.cn/666/665430/665430.mp4
概述Presents a comprehensive review of both the astrophysical nature of individual red dwarf and brown dwarf stars and their collective statistical properties.Revised edition includes important new materi
叢書(shū)名稱Springer Praxis Books
圖書(shū)封面Titlebook: New Light on Dark Stars; Red Dwarfs, Low-Mass I. Neill Reid,Suzanne L. Hawley Book 2005Latest edition Springer-Verlag Berlin Heidelberg 200
描述There has been very considerable progress in research into low-mass stars, brown dwarfs and extrasolar planets during the past few years, particularly since the fist edtion of this book was published in 2000. In this new edtion the authors present a comprehensive review of both the astrophysical nature of individual red dwarf and brown dwarf stars and their collective statistical properties as an important Galactic stellar population. Chapters dealing with the observational properies of low-mass dwarfs, the stellar mass function and extrasolar planets have been completely revised. Other chapters have been significantly revised and updated as appropriate, including important new material on observational techniques, stellar acivity, the Galactic halo and field star surveys. The authors detail the many discoveries of new brown dwarfs and extrasolar planets made since publication of the first edition of the book and provide a state-of-the-art review of our current knowledge of very low-mass stars, brown dwarfs and extrasolar planets, including both the latest observational results and theoretical work.
出版日期Book 2005Latest edition
關(guān)鍵詞dwarf stars; extrasolar planets; low mass stars; star; stellar
版次2
doihttps://doi.org/10.1007/3-540-27610-6
isbn_softcover978-3-642-06418-0
isbn_ebook978-3-540-27610-4
copyrightSpringer-Verlag Berlin Heidelberg 2005
The information of publication is updating

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The mass function,re parameters, such as the local mass density. At present, masses can be derived directly only for stars in binary systems with well-determined orbits, although microlensing projects may offer additional data in the future. Those stars are used to calibrate empirical mass-luminosity relationships, w
地板
發(fā)表于 2025-3-22 06:59:34 | 只看該作者
M dwarfs in the Galactic Halo,n their higher-temperature counterparts, recent theoretical work, both on the atmospheres and on the internal structure, combined with the availability of better data, have opened the way to more quantitative analysis. Abundances can be estimated, both from the location of stars in the H-R diagram a
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發(fā)表于 2025-3-22 08:57:00 | 只看該作者
Extrasolar planets,r techniques, such as photometric transit and microlensing surveys, have recently started to contribute to the planetary census. With ~130 host systems currently known, it is clear that the mass distribution of these very-low mass companions is not an extension of the mass function of stellar/brown
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發(fā)表于 2025-3-22 15:33:25 | 只看該作者
mmungen (z.?B. Landesbauordnung – LBO), d.?h. den einschl?gigen DIN-Vorschriften und sonstiger Richtlinien. Die . selbst dient zum . von Lasten (F?rdertechnik) und ist nicht baugenehmigungspflichtig. Ihre ?Abnahme“ f?llt in den Zust?ndigkeitsbereich der hierfür anerkannten Sachverst?ndigen, welche d
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發(fā)表于 2025-3-22 20:03:25 | 只看該作者
mmungen (z.?B. Landesbauordnung – LBO), d.?h. den einschl?gigen DIN-Vorschriften und sonstiger Richtlinien. Die . selbst dient zum . von Lasten (F?rdertechnik) und ist nicht baugenehmigungspflichtig. Ihre ?Abnahme“ f?llt in den Zust?ndigkeitsbereich der hierfür anerkannten Sachverst?ndigen, welche d
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發(fā)表于 2025-3-23 01:54:40 | 只看該作者
gen. Man denke nur an die Verdrehung l?ngs der Stabachse bei einem Plattenbalken als Randunterstützung einer Platte. Wegen der Verbundwirkung zwischen Platte und Balken muβ der Balken die gleiche Verdrehung haben, wie sie die Platte als Neigung der Tangente an die Biegelinie am Auflager hat. Wie hin
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