obdurate
发表于 2025-3-21 18:27:50
书目名称Dust and Molecules in Evolved Stars影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0283449<br><br> <br><br>书目名称Dust and Molecules in Evolved Stars读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0283449<br><br> <br><br>
jeopardize
发表于 2025-3-21 20:17:23
https://doi.org/10.1007/978-94-017-1307-8Galaxy; Star; astrophysics; cluster; molecule; spectra; stellar
似少年
发表于 2025-3-22 00:33:57
978-90-481-5018-2Springer Science+Business Media Dordrecht 1998
Osmosis
发表于 2025-3-22 07:56:33
Theodore Pelagidis,Michael MitsopoulosIn this contribution, we present a few highlights of the guaranteed time program to observe AGB stars with differing chemical compositions and mass loss rates using ISO . SWS. We briefly discuss C.H. absorption in C-stars and 0-rich stars with the 13 μm dust emission.
产生
发表于 2025-3-22 12:27:46
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ARENA
发表于 2025-3-22 13:18:38
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ARENA
发表于 2025-3-22 17:13:06
IR-Colors for Models of Post-AGB Evolution its effective temperature, .., starts to increase, which soon causes the mass loss rate to decrease significantly. When .. reaches about 30 000 K, the star eventually enters the planetary nebula (PN) phase. The transition from the AGB to the PN stage, believed to last a few thousand years, is called the . phase of evolution.
事先无准备
发表于 2025-3-23 00:00:48
Theodore Pelagidis,Michael Mitsopoulos known features at 3.3, 6.2, 7.7, 8.6, and 11.3 µm a wealth of weaker features is present as well. These studies also reveal detailed variations from source to source, which may be of key importance in the molecular identification process. The emission from Polycyclic Aromatic Hydrocarbon molecules
aesthetician
发表于 2025-3-23 05:04:26
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Immortal
发表于 2025-3-23 07:58:20
Theodore Pelagidis,Michael Mitsopouloslicity of their geometry and kinematics, and the large variety in their physical and chemical (C/O<1 as well as >1) characteristics, make them excellent targets for the study of molecular formation processes. This review presents a compilation of estimated molecular abundances, discusses the uncerta