encomiast
发表于 2025-3-28 16:54:54
J. F. Lancasterursts actually achieve super-Eddington luminosities, and if so, how? (c) What are the characteristics of quasi-static mass loss in the presence of such luminosities? (d) How is the color temperature related to the effective temperature? and, (e) What are the implications concerning the Galactic dist
江湖郎中
发表于 2025-3-28 22:07:27
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地壳
发表于 2025-3-29 01:09:50
J. F. Lancasterrd to find? Why do young stellar objects almost universally exhibit powerful outflows? Why is the geometry for these outflows often bipolar? Why do T Tauri stars have such active chromospheres? In this review we suggest that these puzzles all have a related resolution, in the nature of how gravitati
骑师
发表于 2025-3-29 04:45:54
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手段
发表于 2025-3-29 07:59:08
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CLAY
发表于 2025-3-29 12:27:26
J. F. Lancasterces. The pulsed X-ray emission from the pulsating binary X-ray sources probably comes from “mounds” of accreting gas at the magnetic poles of neutron stars, in which the accreting matter is decelerated by radiation pressure. The physics of these systems is reviewed, with an emphasis on problems for