Extraneous
发表于 2025-3-21 18:56:55
书目名称Stellar Rotation影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0877165<br><br> <br><br>书目名称Stellar Rotation读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0877165<br><br> <br><br>
CHAFE
发表于 2025-3-21 20:32:23
On the Effect of Rotation on Stellar Absorption Lineseric parameters of a rapidly rotating star seen pole-on are very similar to those of a non-rotating star of the same mass, this may cause significant errors in abundance determinations, especially for Eu-type elements. The aspect effect on the central intensity of two EuII lines of different strengths is also studied.
严重伤害
发表于 2025-3-22 03:33:27
Rotation and Macroturbulence in Supergiant Starsportant a broadening agent as large-scale mass motion. In the middle B and A stars turbulence dominates but there still is an appreciable contribution from rotation. (2) In spite of the fact that the stars observed seem to be losing mass, there is no strong evidence for significant angular momentum loss.
GULF
发表于 2025-3-22 05:48:01
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使成核
发表于 2025-3-22 12:08:56
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充气女
发表于 2025-3-22 16:46:22
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PARA
发表于 2025-3-22 20:29:41
Rotational Velocities of Evolved A and F Starstent with the hypothesis of stellar rotation in completely uncoupled shells for stars that have expanded in radius by less than a factor of four. They do, however, support the hypothesis of solid-body rotation for these stars. The data for the giant stars are discussed, but no firm conclusions about
amorphous
发表于 2025-3-22 23:16:17
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GROG
发表于 2025-3-23 01:40:34
Evolution of Rapidly Rotating B-Type Stars and Roxburgh and Strittmatter (1965) how seriously the spectrum of a star may be affected by rotation. However, before atmospheric models for rotating stars can be computed, the results of corresponding interior models have to be available. For polytropic configurations a great many rotating interi
有害
发表于 2025-3-23 08:29:45
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