调停 发表于 2025-3-21 16:57:58

书目名称Late Stages of Stellar Evolution影响因子(影响力)<br>        http://impactfactor.cn/if/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution影响因子(影响力)学科排名<br>        http://impactfactor.cn/ifr/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution网络公开度<br>        http://impactfactor.cn/at/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution网络公开度学科排名<br>        http://impactfactor.cn/atr/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution被引频次<br>        http://impactfactor.cn/tc/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution被引频次学科排名<br>        http://impactfactor.cn/tcr/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution年度引用<br>        http://impactfactor.cn/ii/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution年度引用学科排名<br>        http://impactfactor.cn/iir/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution读者反馈<br>        http://impactfactor.cn/5y/?ISSN=BK0581781<br><br>        <br><br>书目名称Late Stages of Stellar Evolution读者反馈学科排名<br>        http://impactfactor.cn/5yr/?ISSN=BK0581781<br><br>        <br><br>

Highbrow 发表于 2025-3-21 23:21:45

Late Stages of Stellar Evolution978-94-010-2237-8Series ISSN 1743-9213 Series E-ISSN 2352-2186

蘑菇 发表于 2025-3-22 00:58:26

International Astronomical Union Symposiahttp://image.papertrans.cn/l/image/581781.jpg

MULTI 发表于 2025-3-22 08:15:11

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perjury 发表于 2025-3-22 12:13:00

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voluble 发表于 2025-3-22 13:32:47

Mass Ejection by Radiation Pressure, the optically thick regions. There were many attempts to find selfconsistent models of time-independent mass outflow driven by this mechanism (Finzi and Wolf, 1971; Bisnovaty-Kogan and Nadyozhin, 1972; and many others); however, neither was satisfactory.

诱使 发表于 2025-3-22 18:15:16

Nuclear Reactions and Neutrinos in Stellar Evolution,Much of the material discussed in this review represents a summary of some chapters in a monograph I am writing (Arnett, 1974); a more detailed discussion will be found there.

食道 发表于 2025-3-23 01:00:25

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Felicitous 发表于 2025-3-23 02:48:54

Non-Explosive Mass Loss,The various mechanisms whereby stars might lose matter are considered, together with the observational evidence of the mass loss rates associated with these mechanisms. The results are shown in a diagram giving the fractional mass that a star loses by various mechanisms as a function of initial mass.

EPT 发表于 2025-3-23 06:38:36

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查看完整版本: Titlebook: Late Stages of Stellar Evolution; R. J. Tayler,J. E. Hesser Book 1974 International Astronomical Union 1974 gravitation.gravity.planet.sta