厌氧
发表于 2025-3-21 16:49:32
书目名称Cool Stars, Stellar Systems and the Sun影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<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=BK0237887<br><br> <br><br>
ATOPY
发表于 2025-3-22 00:08:03
Correlation of the Mg II h & k flux versus rotational period in late-type stars,otational periods. It is shown that the relationship proposed by Hartmann et al for F to K stars does extend to the dMe stars, although there is more scatter. This is in part due to our inability to use the parameter representing the convective-overturn time.
朴素
发表于 2025-3-22 03:58:44
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DALLY
发表于 2025-3-22 07:58:07
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平庸的人或物
发表于 2025-3-22 09:17:42
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molest
发表于 2025-3-22 16:44:08
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molest
发表于 2025-3-22 19:42:29
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cortex
发表于 2025-3-23 00:40:16
Undesired Effects of Input Saturation,ctral types that, on the basis of current models, correspond to fully convective interiors. Hence, the results support a rotation-dependent distributed dynamo (or some variation thereof) as a viable model for the generation of magnetic flux in the very low mass stars. Future work should include v si
engrossed
发表于 2025-3-23 04:48:03
Correlation of the Mg II h & k flux versus rotational period in late-type stars,otational periods. It is shown that the relationship proposed by Hartmann et al for F to K stars does extend to the dMe stars, although there is more scatter. This is in part due to our inability to use the parameter representing the convective-overturn time.
痛恨
发表于 2025-3-23 07:03:04
Cool Stars, Stellar Systems and the Sun978-3-540-38731-2Series ISSN 0075-8450 Series E-ISSN 1616-6361