The Emission from Post-Shock Flows in mCVs

Details The Emission from Post-Shock Flows in mCVs The Emission from Post-Shock Flows in mCVs

1999-07-21

arxiv.org/abs/astro-ph/9907285v1

Astronomy and Astrophysics

Astrophysics

6 pages, to be published in the Proc of the Symp. to mark the 60th birthday of Brian Warner

Scientific paper

10.1016/S1387-6473(00)00014-2

We re-examine the vertical structure of the post-shock flow in the accretion
region of mCVs, and the X-ray emission as a function of height. We then predict
X-ray light curves and phase-resolved spectra, taking into account the vertical
structure, examine the implications and check whether the predicted heights are
compatible with observation.

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