Confer 发表于 2025-3-21 17:00:13
书目名称Hydrogen Deficient Stars and Related Objects影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0430381<br><br> <br><br>书目名称Hydrogen Deficient Stars and Related Objects读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0430381<br><br> <br><br>cortisol 发表于 2025-3-21 21:29:48
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Hydrogen Deficient Stars and Related Objects978-94-009-4744-3Series ISSN 0067-0057 Series E-ISSN 2214-7985广大 发表于 2025-3-22 08:12:46
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A Preliminary Analysis of the Pulsating Extreme Helium Star V652 Her (Bd+13°3224)A preliminary fine analysis of the atmosphere of the pulsating extreme star V652 Her (=BD+13°3224) is reported. The mean effective temperature and temperature variation have been determined from the ionisation equilibria of Si and N. Both of these elements are strongly overabundant, whilst C appears to be underabundant.Commentary 发表于 2025-3-23 04:23:33
Polarimetric Observations of Hydrogen Deficient StarsPolarimetric observations of HD 30353,SU Tau,XX Cam, R Cr B,UV Cas, BD+13° 3224,BD+10° 2179 and HD 124448 are presented. The linear polarization of HD 30353 is found to vary appreciably at Hα over a time scale as short as one day. It is also found that SU Tau shows significant variation in polarisation even at light maximum.利用 发表于 2025-3-23 07:49:15
Introductory Commentsy unable to attend. This I am happy to do: the hydrogen-deficient stars are dear to my heart and even though I haven’t contributed anything to the subject for several years, it is certainly nice to be remembered. From an outsider, then, a few thoughts.