X-ray emission from cataclysmic variables with accretion disks. II. EUV/Soft x-ray radiation

Keywords

Physics, Astrophysics, White dwarf, Cataclysmic variable star, Accretion (finance)

References

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Cited by

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• SWIFT OBSERVATIONS OF HARD X-RAY EMITTING WHITE DWARFS IN SYMBIOTIC STARSJ. A. Kennea, K. Mukai, J. L. Sokoloski — 2009
• The ROSAT view of the cataclysmic variable skyK. Beuermann, H. C. Thomas — 1993
• X-ray variations in the inner accretion flow of Dwarf NovaeŞ. Balman, M. Revnivtsev — 2012
• X-RAY AND ULTRAVIOLET EMISSION FROM THE RECURRENT NOVA RS OPHIUCHI IN QUIESCENCE: SIGNATURES OF ACCRETION AND SHOCKED GASThomas Nelson, K. Mukai, Marina Orio — 2011
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• Modeling the EUV spectra of optically thick boundary layers of dwarf novae in outburstV. Suleimanov, M. Hertfelder, K. Werner — 2014
• Hydrodynamic Simulations of Flares on Accretion DisksGlen Williams, Kerriann H. Malatesta — 2002
• Hard X-rays from accretion disk boundary layersRamesh Narayan, Robert Popham — 1993

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