CHORD
发表于 2025-3-21 16:56:11
书目名称Cool Stars, Stellar Systems, and the Sun影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0237889<br><br> <br><br>书目名称Cool Stars, Stellar Systems, and the Sun读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0237889<br><br> <br><br>
backdrop
发表于 2025-3-21 23:33:29
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人类
发表于 2025-3-22 02:20:08
978-3-540-12907-3Springer-Verlag Berlin Heidelberg 1984
Crumple
发表于 2025-3-22 05:24:51
Khaled Khelif,Rose Dieng-Kuntz,Pascal Barbry chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations of T Tauri activity can be linked to vigorous solar-stellar phenomena characteristic of cool stars of low mass, other characteristics of T Tauri behavior are exhibited by a wide ran
小步舞
发表于 2025-3-22 10:54:09
Mike Dean,Yuanbo Guo,Quan Z. Shengncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
性行为放纵者
发表于 2025-3-22 13:25:18
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性行为放纵者
发表于 2025-3-22 17:35:21
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倾听
发表于 2025-3-23 00:56:47
W. M. P. van der Aalst,M. Pesicquence is given. From stars of main-sequence spectral type A through early K, the dependence of rotation on mass and age is investigated, from results for stars in open clusters and in the field. The high-mass, single, normal dwarf stars of spectral type A display a common mean projected rotational
beta-cells
发表于 2025-3-23 05:24:31
Cool Stars, Stellar Systems, and the Sun978-3-540-38785-5Series ISSN 0075-8450 Series E-ISSN 1616-6361
Bph773
发表于 2025-3-23 05:36:16
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