EWE 发表于 2025-3-28 14:55:42
Can ultrarelativistic neutrons from the central engine drive the outflow in broad absorption line Qing gas has to be sufficiently low for it to remain cool, which requires that the wind is very efficiently heated by the ultrarelativistic protons. This could be accomplished through the excitation and subsequent damping of Alfvén waves, or by a turbulent wind structure containing shocks that will darsenal 发表于 2025-3-28 20:24:48
http://reply.papertrans.cn/83/8263/826219/826219_42.pngoutput 发表于 2025-3-28 23:01:12
http://reply.papertrans.cn/83/8263/826219/826219_43.png闪光东本 发表于 2025-3-29 04:58:58
Influence of Second-Order Fermi acceleration and Relativistic Shock Waves on Nonthermal Continuum Ewaves are not able to generate cut-offs which are steep enough to fit the observed spectra. The reason is the fact that we usually only see the part of the anisotropic spectrum in optically thin sources directed towards us and therefore at small pitch angles. But at small pitch angles cutoffs are lecutlery 发表于 2025-3-29 09:29:11
http://reply.papertrans.cn/83/8263/826219/826219_45.png伴随而来 发表于 2025-3-29 13:29:45
Lecture Notes in Physicshttp://image.papertrans.cn/r/image/826219.jpgnostrum 发表于 2025-3-29 16:27:12
https://doi.org/10.1007/3-540-54789-4Astrophysik; Neutron; accretion; cosmic compact objects; cosmic rays; electron-positron pair production; hExternalize 发表于 2025-3-29 20:37:03
http://reply.papertrans.cn/83/8263/826219/826219_48.png不来 发表于 2025-3-30 03:53:14
http://reply.papertrans.cn/83/8263/826219/826219_49.pngConclave 发表于 2025-3-30 05:49:20
978-3-662-13823-6Springer-Verlag Berlin Heidelberg 1991