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September 17, 2012Astronomy and AstrophysicsOpen Access

X-ray variations in the inner accretion flow of dwarf novae

Ş. Balman M. Revnivtsev

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Abstract

Aims. We study the inner disk structure of dwarf novae (DNe; i.e., nonmagnetic cataclysmic variables).

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Cite This Study

Balman et al. (2012) studied this question.

synapsesocial.com/papers/6a841a9d25efb1e71e83da67 https://doi.org/10.1051/0004-6361/201219469

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