Jejunum
发表于 2025-3-21 17:52:12
书目名称Stellar Astrophysics影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0877147<br><br> <br><br>书目名称Stellar Astrophysics读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0877147<br><br> <br><br>
学术讨论会
发表于 2025-3-21 20:19:44
Gamma-Ray Pulsars in Gould Belt and Unidentified Gamma-Ray Sources in Medium Latitudes can exist even their age > 10. yr old. We use Monte Carlo techniques to simulate the statistical properties of rotation-powered pulsars in the Gould Belt. If the pulsar birth rate in Gould Belt is 3 × 10..., the gamma-ray pulsars in this region, which can be detected by EGRET, will must be dominate
misanthrope
发表于 2025-3-22 01:55:04
Magnetars and Pulsars: A Missing Link fields, i.e., magnetars, marking them a distinguished species from the conventional species of spindown-powered isolated neutron stars, i.e., radio pulsars. The current arguments in favor of the magnetar interpretation of SGR/AXP phenomenology will be outlined, and the two energy sources in magneta
西瓜
发表于 2025-3-22 05:07:26
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流利圆滑
发表于 2025-3-22 09:35:22
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假装是我
发表于 2025-3-22 13:59:16
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Inflated
发表于 2025-3-22 18:11:39
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PURG
发表于 2025-3-23 00:16:52
Phase Transition in Rotating Hybrid Starsmoment of inertia, and even results in an era of spin-up of the pulsar (Glendenning, Pei, & Weber 1997, hereafter GPW) . We have found that the equation of states of the crust of neutron star and the accuracy of the numerical models which can be used to determinate the stellar rotating properties ar
Lipohypertrophy
发表于 2025-3-23 03:06:55
Accretion Disk Oscillations and QPOs in X-Ray Binariesation modes in a relativistic accretion disk. Here we studied the non-damping feature of some oscillation modes by considering the radial perturbations and viscosity effects. We found that the non-damping fundamental modes can be amplified significantly in the inner disk when the viscosity parameter
charisma
发表于 2025-3-23 09:29:32
Bare Strange Quark Stars: Formation and Emissionmperature after the supernova detonation flame, and a crust can also hardly form except for a super-Eddington accretion. The magnetosphere of a bare strange star is composed mainly of e. pair plasma, where both inner and outer vacuum gaps work for radio as well as high energy nonthermal emission. A