F. Bernardini, Domitilla de Martino, M. Falanga, K. Mukai, G. Matt, J. M. Bonnet-Bidaud, Nicola Masetti, M. Mouchet
Abstract
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Aims. We aim at characterizing a sample of nine new hard X-ray selected cataclysmic variable (CVs), to unambiguously identify them as magnetic systems of the intermediate polar (IP) type.
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Aims. We aim at characterizing a sample of nine new hard X-ray selected cataclysmic variable (CVs), to unambiguously identify them as magnetic systems of the intermediate polar (IP) type.
Key concepts: White dwarf, Physics, Cataclysmic variable star, Astrophysics, Intermediate polar, X-ray, Orbital period, Spectral line