可扩大
发表于 2025-3-21 19:39:34
书目名称Observational Evidence for Black Holes in the Universe影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0700361<br><br> <br><br>书目名称Observational Evidence for Black Holes in the Universe读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0700361<br><br> <br><br>
大沟
发表于 2025-3-21 21:37:02
Accretion Disks around Black Holes: Twenty Five Years Later,te in the form of accretion disks were put forward (Burbidge . Prendergast, 1968; Lynden-Bell, 1969). More quantitative studies were made by Shakura (1972). However, the beginning of modern accretion disk physics is traditionally attributed to the two classical articles, one by Shakura & Sunyaev (19
irritation
发表于 2025-3-22 02:33:58
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同步左右
发表于 2025-3-22 06:51:08
Simulations of Shocks with Smoothed Particles Hydrodynamics Method, the last few years through numerical simulations by a novel technique named Smoothed Particles Hydrodynamics (SPH). We concentrate on the axisymmetric problems which are done using cylindrical coordinates. The plan of this contribution is the following: in Section 2 we describe the SPH numerical me
Seminar
发表于 2025-3-22 12:42:29
Nucleosynthesis in Advective Accretion Disks around Galactic and Extra-Galactic Black Holes,barti, 1998). Earlier works have been done in cooler thick accretion disks only. Below, we present a few examples of nuclear reactions in advective flows and discuss the implications. Results of more detailed study could be seen in Mukhopadhyay & Chakrabarti (1998) .
Innocence
发表于 2025-3-22 13:59:51
Computation of Mass-Outflow Rates from Advective Accretion Disks around Black Holes,MRC96; Ryu, Chakrabarti & Molteni, 1997; Nobuta & Hanawa, 1998). ¿ From the analytical front, although the wind type solutions and accretion type solutions come out of the same set of governing equations (Chakrabarti 1990), there are few, and mostly qualitative attempt to find connections among them
Anthrp
发表于 2025-3-22 20:43:44
High Energy Gamma-Ray Emission from Blazars: ,,ted particles, γ-ray emission is believed to be due to inverse Compton scattering of low energy photons, although opinions differ as to the source of the soft photons. Hardronic models involve secondary production or photomeson production followed by pair cascades, and predict associated neutrino pr
防水
发表于 2025-3-23 00:44:08
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TOXIN
发表于 2025-3-23 01:28:35
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贿赂
发表于 2025-3-23 07:03:14
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