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Article overview
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X-ray Spectroscopy of Cataclysmic Variables | Koji Mukai
; | Date: |
3 Dec 2001 | Subject: | astro-ph | Affiliation: | NASA/GSFC and Usra | Abstract: | In cataclysmic variables (CVs), accretion onto white dwarfs produces high temperature, high density plasmas. They cool down from kT~10 keV via bremsstrahlung continuum and K and L shell line emissions. The small volume around white dwarfs means that the plasma densities are much higher than in, e.g., stellar coronae, probably beyond the range well-described by existing models. I will describe potential diagnostics of the temperatures, the densities, and the optical depths of X-ray emitting plasmas in CVs, and present the recent Chandra grating spectra of the magnetic CV V1223 Sgr as an example. | Source: | arXiv, astro-ph/0112048 | Services: | Forum | Review | PDF | Favorites |
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