deliberate 发表于 2025-3-21 19:54:17
书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0188947<br><br> <br><br>书目名称Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0188947<br><br> <br><br>palliative-care 发表于 2025-3-22 00:17:06
http://reply.papertrans.cn/19/1890/188947/188947_2.png金盘是高原 发表于 2025-3-22 02:01:10
,Theorien zu Unternehmensübernahmen,ll stellar motions are very close to isotropy. They indicate a central mass concentration with a density . M. pc. that dominates the potential between 0.01 and 1 pc. The derived mass ranges between 2.6 and 3.3 x 10. M. for a distance of 8.0 kpc. Such a mass concentration cannot be stable and must be催眠 发表于 2025-3-22 05:22:21
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http://reply.papertrans.cn/19/1890/188947/188947_6.pngagonist 发表于 2025-3-22 20:42:57
Hans-Gert Penzel,Christian PietigThe maximum mass of neutron stars is one of the most important predictions of the general relativistic theory of stellar structure. This paper highlights the difficulties in making a definitive prediction, and also reviews the progress made so far.摇曳的微光 发表于 2025-3-23 00:59:02
David Fubini,Colin Price,Maurizio ZolloThe advent of the large effective apertures of the Keck telescopes has resulted in the determination with unprecedented accuracy of the mass functions and mass ratios of faint (. mag) X-ray transients (GS 2000+25, GRO J0422+32, Nova Oph 1977, Nova Vel 1993).ILEUM 发表于 2025-3-23 03:24:52
http://reply.papertrans.cn/19/1890/188947/188947_9.png全部逛商店 发表于 2025-3-23 05:47:28
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