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发表于 2025-3-21 18:14:23
书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0625307<br><br> <br><br>书目名称Mass-Losing Pulsating Stars and their Circumstellar Matter读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0625307<br><br> <br><br>
狗舍
发表于 2025-3-21 20:42:47
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agenda
发表于 2025-3-22 03:47:32
Luminosities of AGB Variabless in the LMC and galactic globular clusters. Hipparcos observations indicate that most Miras in the solar neighbourhood are consistent with such a relation. There are two groups of stars with luminosities that are apparently greater than the PL relation would predict: (1) in the LMC and SMC there ar
火花
发表于 2025-3-22 07:47:24
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COUCH
发表于 2025-3-22 12:08:35
Stellar Sources in the Isogal Intermediate Bulge Fields In combination with near-infrared (IJK.) data of DENIS survey, we discuss the nature of the ISOGAL sources, their luminosities, the interstellar extinction and the mass-loss rates. A large fraction of the detected sources at 15 . are AGB stars above the RGB tip, a number of them show an excess in (
尖叫
发表于 2025-3-22 15:25:21
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promote
发表于 2025-3-22 18:17:56
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偏狂症
发表于 2025-3-22 22:15:05
Nonlinear Properties of the Semi-Regular Variable Starsulsation mechanism. An application to R Sct thus shows that the irregular lightcurve is the result of the nonlinear interaction of two highly nonadiabatic pulsation modes, namely a linearly unstable, low frequency mode, and the second mode that, although linearly stable, gets entrained through a 2:1
人工制品
发表于 2025-3-23 04:54:28
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LINES
发表于 2025-3-23 05:44:17
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