废墟 发表于 2025-3-28 18:18:45
http://reply.papertrans.cn/15/1438/143796/143796_41.pngEvacuate 发表于 2025-3-28 20:42:11
http://reply.papertrans.cn/15/1438/143796/143796_42.pngETHER 发表于 2025-3-29 01:18:49
Gillian Morrison,Joshua M. Tobinnecessarily coplanar with the disc midplane..The calculations are relevant to a number of observed astrophysical phenomena, including the precession of jets associated with young stars, the high spectral index of some T Tauri stars, and the light curves of X-ray binaries such as Hercules X-1 which sA保存的 发表于 2025-3-29 06:26:39
http://reply.papertrans.cn/15/1438/143796/143796_44.png6Applepolish 发表于 2025-3-29 07:31:15
http://reply.papertrans.cn/15/1438/143796/143796_45.png破裂 发表于 2025-3-29 14:27:50
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Jennifer Cone,Demetrios Demetriadesgenerally possess a sub-Keplerian angular momentum distribution and have maximum temperatures in the range 10. – 10. K. Accretion discs around rotating black holes are hotter and deposit less angular momentum on the central object than accretion discs around Schwarzschild black holes.讨好女人 发表于 2025-3-30 03:28:24
http://reply.papertrans.cn/15/1438/143796/143796_49.pngendocardium 发表于 2025-3-30 04:56:48
Anatomy of the Subaxial Cervical Spineal and short term variability characteristics of the hard X-ray emission were observed in the low spectral state of several black hole binaries. Possible relation of these variations with change of the mass accretion rate and low/high spectral state transitions is discussed.