Titlebook: Observational Evidence for Black Holes in the Universe; Proceedings of a Con Sandip K. Chakrabarti Conference proceedings 1999 Springer Sci

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書目名稱Observational Evidence for Black Holes in the Universe影響因子(影響力)




書目名稱Observational Evidence for Black Holes in the Universe影響因子(影響力)學(xué)科排名




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書目名稱Observational Evidence for Black Holes in the Universe被引頻次學(xué)科排名




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書目名稱Observational Evidence for Black Holes in the Universe年度引用學(xué)科排名




書目名稱Observational Evidence for Black Holes in the Universe讀者反饋




書目名稱Observational Evidence for Black Holes in the Universe讀者反饋學(xué)科排名

大溝

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

同步左右

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

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) [MC98].

Innocence

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

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

TOXIN

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