Titlebook: Relativistic Hadrons in Cosmic Compact Objects; Proceedings of a Wor Andrzej A. Zdziarski,Marek Sikora Conference proceedings 1991 Springer

EWE

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 d

arsenal

output

闪光东本

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 le

cutlery

伴随而来

Lecture Notes in Physicshttp://image.papertrans.cn/r/image/826219.jpg

nostrum

https://doi.org/10.1007/3-540-54789-4Astrophysik; Neutron; accretion; cosmic compact objects; cosmic rays; electron-positron pair production; h

Externalize

不来

Conclave

978-3-662-13823-6Springer-Verlag Berlin Heidelberg 1991