Effect of the reverse shock on the parameters of the observed X-Ray emission during the 1998 outburst of CI Cam


Based on the model of interaction between spherically symmetrical expanding matter and the external medium, we have estimated the parameters of the matter heated by the shock that was produced in the envelope ejected by the explosion of a classical nova during its interaction with the stellar wind from the optical companion. Using this model, we have shown… (More)


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