fungus
发表于 2025-3-21 16:21:50
书目名称Kinematics and Dynamics of Diffuse Astrophysical Media影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0543024<br><br> <br><br>书目名称Kinematics and Dynamics of Diffuse Astrophysical Media读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0543024<br><br> <br><br>
BRAWL
发表于 2025-3-21 22:50:00
Parametric determination of the inclination of Keplerian circumstellar discs from spectropolarimetrcircumstellar disc are presented. It is shown that analysis of the scattered line profiles at different wavelengths which, due to Doppler redistribution, sample different disc regions allows the disc inclination to be determined.
crescendo
发表于 2025-3-22 03:07:45
Jets,s. Recent measurements of the proper motions of HH objects show that even those near the source are moving at about the same speed as the jet fluid. This means that they cannot be due to steady shocks in the jet and the only obvious explanation is that the source is varying.
Panacea
发表于 2025-3-22 04:45:17
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outrage
发表于 2025-3-22 09:33:15
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backdrop
发表于 2025-3-22 13:32:37
Cosmical Gas Dynamics, Why Was It So Difficult?,When the invitation for this meeting reached me, I did not hesitate. Of course, I wished to be present when it was Franz Kahn’s turn for the formal move to say goodbye. Like many of us, he will probably sneak in again through the back door and continue working.
把…比做
发表于 2025-3-22 19:44:20
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Obliterate
发表于 2025-3-22 23:03:05
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暂时休息
发表于 2025-3-23 05:27:06
Complex Structure Associated with the Wolf-Rayet Star WR147,The Wolf-Rayet star WR147 is known to be bright at X-ray and radio wavelengths (van der Hucht ., 1981, Caillaut ., 1985, Abbot ., 1986).
产生
发表于 2025-3-23 08:46:08
The Importance of Continuum Radiation for the Stellar Wind Hydrodynamics of Hot Stars,The contribution of bound-free and free-free processes to the outward acceleration of ζPup is studied and is found to be negligible.