NK871
发表于 2025-3-21 16:51:00
书目名称Evolution of Massive Stars影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0317744<br><br> <br><br>书目名称Evolution of Massive Stars读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0317744<br><br> <br><br>
痛苦一生
发表于 2025-3-21 23:49:25
Das Systemisch-integrative Führungsmodell derived for O—stars show, in general terms, good agreement with predictions from the latest radiation—driven wind models, although some discrepancies are apparent. Several LBVs show similar mass-loss rates at maximum and minimum states, contrary to previous expectations, with the mechanism responsi
Hyperopia
发表于 2025-3-22 02:24:35
Book 1994olution therefore got a chance in these meetings, but rarely as a prime subject. The state of the art, the physical processes and the uncertainties in stellar evolution were barely touched. Even more, the influence of close binaries in all these massive star meetings slowly disappeared the last, say
separate
发表于 2025-3-22 05:06:52
ve star evolution therefore got a chance in these meetings, but rarely as a prime subject. The state of the art, the physical processes and the uncertainties in stellar evolution were barely touched. Even more, the influence of close binaries in all these massive star meetings slowly disappeared the last, say978-94-010-4471-4978-94-011-1080-8
FLOUR
发表于 2025-3-22 11:13:25
Spectral Synthesis of Spectral Populations using Balmer Linesalaxies. The colors of a young starburst as well as most of its spectral features are relatively unaffected by stars of a few solar masses which contribute little to the integrated luminosity and to the ionization and excitation properties. However, as the Balmer lines are much stronger for those st
慷慨不好
发表于 2025-3-22 13:16:34
Observations of the Atmospheres and Winds of O-stars, LBVs and Wolf-Rayet Stars derived for O—stars show, in general terms, good agreement with predictions from the latest radiation—driven wind models, although some discrepancies are apparent. Several LBVs show similar mass-loss rates at maximum and minimum states, contrary to previous expectations, with the mechanism responsi
慷慨不好
发表于 2025-3-22 19:07:10
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变化
发表于 2025-3-23 00:34:24
Erfolg als theoriegeleitete Kategorie,the SMC are 185, 114, and 9, respectively. Distances and galactic distributions determined by various authors are compared. The single star and binary distributions are discussed in the light of evolutionary studies.
不遵守
发表于 2025-3-23 01:44:07
https://doi.org/10.1007/978-3-531-93479-2method to account for the huge number of atomic levels and line transitions is presented. Results of exploratory model calculations examining the effects on the temperature structure, the hydrogen and helium line profiles and UV/EUV fluxes are discussed.
AXIOM
发表于 2025-3-23 08:31:59
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