Effect of the reverse shock on the parameters of the observed X-Ray emission during the 1998 outburst of CI Cam - Astrophysics > High Energy Astrophysical PhenomenaReportar como inadecuado




Effect of the reverse shock on the parameters of the observed X-Ray emission during the 1998 outburst of CI Cam - Astrophysics > High Energy Astrophysical Phenomena - Descarga este documento en PDF. Documentación en PDF para descargar gratis. Disponible también para leer online.

Abstract: Based on the model of interaction between spherically symmetrical expandingmatter and the external medium, we have estimated the parameters of the matterheated by the shock that was produced in the envelope ejected by the explosionof a classical nova during its interaction with the stellar wind from theoptical companion. Using this model, we have shown that the matter ejectedduring the outburst in the system CI Cam had no steep velocity gradients andthat the reverse shock could heat the ejected matter only to a temperature of~0.1 keV. Therefore, this matter did not contribute to the mean temperature andluminosity of the system observed in the energy range 3-20 keV.



Autor: E. V. Filippova 1,2, M. G. Revnivtsev 1,3, A. A. Lutovinov 1 1 Space Research Institute IKI, Moscow, Russia, 2 MPA, Garching-bei-

Fuente: https://arxiv.org/



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