不服从
发表于 2025-3-21 17:00:23
书目名称B Stars影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0180175<br><br> <br><br>书目名称B Stars读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0180175<br><br> <br><br>
committed
发表于 2025-3-21 20:51:54
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打折
发表于 2025-3-22 03:30:10
978-90-481-5080-9Springer Science+Business Media B.V. 1998
Highbrow
发表于 2025-3-22 06:31:47
B Stars978-94-015-9014-3Series ISSN 0067-0057 Series E-ISSN 2214-7985
小故事
发表于 2025-3-22 11:03:30
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cumulative
发表于 2025-3-22 14:07:48
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ACME
发表于 2025-3-22 19:13:32
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muster
发表于 2025-3-22 23:57:28
The Self Absorption Curve Method for the Analysis of Emission Lines of Complex Ions as a Diagnostic tellar envelope. Information can be obtained notably about the excitation conditions, the column density and the dimensions of the line emitting region, without making detailed model dependent complex radiative transfer computations. This method is particularly useful in the study of B star envelopes.
Alpha-Cells
发表于 2025-3-23 02:02:43
The High Excitation Fe II Lines as a Diagnostics of the Outer Envelopes of Early Type Emission Line malously high intensities. We illustrate the case of the high excitation Fe . lines observed in the ultraviolet and near—IR of different stellar categories, and discuss the information which can be derived from their study.
杠杆
发表于 2025-3-23 08:53:01
Rapid Spectral Variability and Spatial and Kinematical Structure of Circumstellar Envelopes of Some tellar envelopes around peculiar Ae/Be stars. The method involved is based on a search for rapid line-profile variability of lines originating in different circumstellar regions. Analysis of these variations opens the way for reconstructing the density and velocity distributions throughout the envelope.