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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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樓主: 可擴(kuò)大
31#
發(fā)表于 2025-3-26 21:18:17 | 只看該作者
A. M. Ghez,B. L. Klein,M. Morris,E. E. Becklin—is one of the most noteworthy examples. However, labor relations in the auto industry are still characterized by considerable conflict, as the 1984 pact was reached only after corporate threats and a strike by the UAW. The goal of this essay is to explain the shift toward more cooperative labor rel
32#
發(fā)表于 2025-3-27 03:53:48 | 只看該作者
Observational Evidence for Black Holes in the UniverseProceedings of a Con
33#
發(fā)表于 2025-3-27 08:18:49 | 只看該作者
Accretion Disc Theory: From the Standard Model until Advection, the sides of the disc. One of the most important new invention of this theory was a phenomenological treatment of the turbulent viscosity, known as “alpha” prescription, when the (r?) component of the stress tensor was approximated by (. P) with a unknown constant a. This prescription played the ro
34#
發(fā)表于 2025-3-27 11:14:58 | 只看該作者
35#
發(fā)表于 2025-3-27 13:47:25 | 只看該作者
Viscosity in Accretion Disks, the presence of even a modicum of angular momentum in the accreting fluid, the strength of the viscosity will have a substantial influence upon the structure of the accretion disk. Unfortunately, under nearly all astrophysically relevant circumstances, all of the well understood microscopic transve
36#
發(fā)表于 2025-3-27 19:09:18 | 只看該作者
37#
發(fā)表于 2025-3-28 02:00:17 | 只看該作者
38#
發(fā)表于 2025-3-28 02:57:55 | 只看該作者
39#
發(fā)表于 2025-3-28 09:23:24 | 只看該作者
Nucleosynthesis in Advective Accretion Disks around Galactic and Extra-Galactic Black Holes, T. ~ 10. °. (Rees, 1984). This flow is usually cooled down through bremsstrahlung and Comptonization effects and hard and soft states are produced depending on the degree by which this cooling takes place (Chakrabarti & Titarchuk, 1995). The generally sub-Keplerian, advective flow after deviating f
40#
發(fā)表于 2025-3-28 12:17:17 | 只看該作者
Computation of Mass-Outflow Rates from Advective Accretion Disks around Black Holes,e types. The first type of solutions confine themselves to the jet properties only, completely decoupled from the internal properties of accretion disks (see, e.g., Begelman, Blandford & Rees, 1984). In the second type, efforts are made to correlate the internal disk structure with that of the outfl
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