KEN
发表于 2025-3-21 17:02:56
书目名称Mass Outflows from Stars and Galactic Nuclei影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0625246<br><br> <br><br>书目名称Mass Outflows from Stars and Galactic Nuclei读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0625246<br><br> <br><br>
Modify
发表于 2025-3-21 21:49:17
Requirements for Theoretical Models of Outflowsd indisputable evidence for mass loss from the α Her system, the topic of mass loss has grown to be a major research area in astrophysics. The review papers presented at this Workshop summarize the current status of this field.
影响
发表于 2025-3-22 01:17:32
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Judicious
发表于 2025-3-22 08:08:10
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Commission
发表于 2025-3-22 09:52:03
Masses of Planetary Nebulae and their Central Starsosity)..The central star mass can only be determined at present from its luminosity and evolutionary considerations. The present status is summarized. A range of masses between 0.5 and 1M are found. Some inconsistancies between theory and observations are discussed.
努力赶上
发表于 2025-3-22 16:36:26
Mass Loss and Post-Asymptotic Giant-Branch Evolutionremnant depends very sensitively on the initial condition prevailing during its formation. By this very reason the somewhat approximative calculations of Paczynski (1971) failed to give a satisfactory explanation of the evolution of the central stars (CPN).
陶器
发表于 2025-3-22 19:26:49
0067-0057 ects, occurring on different scales and at various evolutionary phases, and to discuss the impact of observations from future space missions. For the stars, we thought to follow throughout the evolution the relevance (rates and dynamical rrodes) of the mass loss phenomenon, e. g. to explain how and
安定
发表于 2025-3-23 00:10:22
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synchronous
发表于 2025-3-23 02:49:58
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Arbitrary
发表于 2025-3-23 06:06:28
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