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2005MNRAS.359.1531E - Mon. Not. R. Astron. Soc., 359, 1531-1536 (2005/June-1)
HT Camelopardalis: the simplest intermediate polar spin pulse.
EVANS P.A. and HELLIER C.
Abstract (from CDS):
We suggest that the lack of opacity in the accretion columns of HT Cam, and also of EX Hya and V1025 Cen, results from a low accretion rate owing to their being below the cataclysmic variable period gap.
Abstract Copyright: 2005 RAS
Journal keyword(s): accretion, accretion discs - stars: individual: HT Cam (RXJ0757.0+6306) - novae, cataclysmic variables - X-rays: binaries
Simbad objects: 9
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