標(biāo)題: Titlebook: New Light on Dark Stars; Red Dwarfs, Low-Mass I. Neill Reid,Suzanne L. Hawley Book 2005Latest edition Springer-Verlag Berlin Heidelberg 200 [打印本頁(yè)] 作者: coherent 時(shí)間: 2025-3-21 18:37
書目名稱New Light on Dark Stars影響因子(影響力)
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書目名稱New Light on Dark Stars網(wǎng)絡(luò)公開度學(xué)科排名
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書目名稱New Light on Dark Stars讀者反饋
書目名稱New Light on Dark Stars讀者反饋學(xué)科排名
作者: 固定某物 時(shí)間: 2025-3-22 00:10 作者: Genistein 時(shí)間: 2025-3-22 01:07
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作者: patriarch 時(shí)間: 2025-3-22 06:59
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作者: BIAS 時(shí)間: 2025-3-22 08:57
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 作者: 連系 時(shí)間: 2025-3-22 15:33
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作者: 同來核對(duì) 時(shí)間: 2025-3-22 20:03
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作者: 幾何學(xué)家 時(shí)間: 2025-3-22 23:15 作者: Gudgeon 時(shí)間: 2025-3-23 01:54
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作者: 疏遠(yuǎn)天際 時(shí)間: 2025-3-23 06:22 作者: adipose-tissue 時(shí)間: 2025-3-23 09:43 作者: Entrancing 時(shí)間: 2025-3-23 15:43
I. Neill Reid,Suzanne L. HawleyPresents 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作者: assent 時(shí)間: 2025-3-23 19:08
Springer Praxis Bookshttp://image.papertrans.cn/n/image/665430.jpg作者: 圣人 時(shí)間: 2025-3-23 23:27 作者: 懸掛 時(shí)間: 2025-3-24 03:16 作者: Delude 時(shí)間: 2025-3-24 07:51
Astronomical concepts,es of low-mass dwarfs described in the following chapters:.The aim has been to provide a broad overview rather than a rigorous development, emphasising aspects which are of most practical use to the astronomical observer. More extensive discussions of each of these topics are included amongst the literature cited in the appended bibliography.作者: nocturnal 時(shí)間: 2025-3-24 12:10 作者: curriculum 時(shí)間: 2025-3-24 18:52 作者: BLANC 時(shí)間: 2025-3-24 21:25 作者: BAIT 時(shí)間: 2025-3-25 01:48 作者: 恃強(qiáng)凌弱的人 時(shí)間: 2025-3-25 04:46
The mass function,cting that variations in the form of Ψ.(.) occur from one star-forming region to another. The strongest support for this hypothesis comes from comparing observations of dense, populous clusters, such as Orion and IC 348, against the low-density star-forming clouds in the Taurus-Auriga association. S作者: AWL 時(shí)間: 2025-3-25 07:57
M dwarfs in the Galactic Halo, and is poorly approximated as a power law. Current results in this area are at best provisional. Despite these uncertainties, however, and even given the current low-accuracy abundance estimates, we can use late-type subdwarfs as calibrators in main sequence fitting. The initial results from that a作者: Anticonvulsants 時(shí)間: 2025-3-25 13:10
Extrasolar planets, are that gas giants form more readily at super-solar metallicities, although ～5% of sun-like stars have detectable companions. Lower mass stars also have planetary companions, as emphasised by the discovery of planets around Gl 876 and Gl 836, although the overall frequency of Jovian-mass gas giant作者: 準(zhǔn)則 時(shí)間: 2025-3-25 15:48
Book 2005Latest editionst 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.作者: Legion 時(shí)間: 2025-3-25 20:42
rfs 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.978-3-642-06418-0978-3-540-27610-4作者: 防止 時(shí)間: 2025-3-26 00:46 作者: Intervention 時(shí)間: 2025-3-26 04:32 作者: needle 時(shí)間: 2025-3-26 12:15 作者: 顛簸地移動(dòng) 時(shí)間: 2025-3-26 15:30 作者: Autobiography 時(shí)間: 2025-3-26 18:25
onssteifigkeit für die Standfestigkeit des Bautei — les von wesentlichem Einfluβ ist, muβ die Aufnahme der Torsionsspannungen durch eine entsprechende Stahl — Bewehrung nachgewiesen werden. Zum Beispiel bei einzelnen Plattenbalken, die halbseitig belastet werden k?nnen作者: Tailor 時(shí)間: 2025-3-26 22:17
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