Gratification 发表于 2025-3-21 18:44:03

书目名称Upper Main Sequence Stars with Anomalous Abundances影响因子(影响力)<br>        http://impactfactor.cn/if/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances影响因子(影响力)学科排名<br>        http://impactfactor.cn/ifr/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances网络公开度<br>        http://impactfactor.cn/at/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances网络公开度学科排名<br>        http://impactfactor.cn/atr/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances被引频次<br>        http://impactfactor.cn/tc/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances被引频次学科排名<br>        http://impactfactor.cn/tcr/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances年度引用<br>        http://impactfactor.cn/ii/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances年度引用学科排名<br>        http://impactfactor.cn/iir/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances读者反馈<br>        http://impactfactor.cn/5y/?ISSN=BK0943809<br><br>        <br><br>书目名称Upper Main Sequence Stars with Anomalous Abundances读者反馈学科排名<br>        http://impactfactor.cn/5yr/?ISSN=BK0943809<br><br>        <br><br>

CAJ 发表于 2025-3-21 23:56:23

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轻浮女 发表于 2025-3-22 01:10:48

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RENIN 发表于 2025-3-22 05:42:31

The Magnetic Field and other Parameters of the Chemically Peculiar Starsson it is natural that different investigators are interested in working out and improving methods of determination of B.. Especially great attention attracts the method based on using the multicolor Geneva photometry . Cramer and Maeder have found a dependence between B. and parameter Z of multi

LAST 发表于 2025-3-22 11:04:27

Does ν Cep Indicate a Non-axisymmetric Dynamo?ws a period of about 5 years. It is unplausible that this magnetic field is a relic since νCep was formed by expansion of a B-star. We claim here that νCep represents a dynamo exciting a magnetic field which in the average strongly deviates from symmetry about the rotation axis.

经典 发表于 2025-3-22 16:58:44

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tympanometry 发表于 2025-3-22 21:06:10

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Ptsd429 发表于 2025-3-22 22:14:30

Missing Levels and Lines of Astrophysical Importance and singly ionized atoms and t o gi ve rough predictions of missing levels and lines. The amount of data that have been published for these elements after the edition of the Multiple Tables are considerable. For detailed information about sources of new data and compilations the reader is referred

痴呆 发表于 2025-3-23 04:18:07

Characteristic Absorption Features in the Spectra of Ap-Si Stars Between 1250 and 1850 Åssible. The contribution of the Si II multiplets is calculated in LTE for a typical overabundance x 10. of silicon. It accounts for only a small part of the observed absorption. Common unidentified structures, smaller than the 1400 Å depression are pointed out.

受人支配 发表于 2025-3-23 08:37:36

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查看完整版本: Titlebook: Upper Main Sequence Stars with Anomalous Abundances; Proceedings of the 9 C. R. Cowley,M. M. Dworetsky,C. Mégessier Conference proceedings