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New X-ray observations of the old nova CP Puppis and of the more recent nova V351 Pup
M. Orio, K. Mukai, A. Bianchini +2
We present X-ray observations of the field containing Nova Puppis 1942 (CP Pup) and Nova Puppis 1991 (V351 Pup), done with ASCA in 1998, and with XMM-Newton in 2005. The X-ray and…
Orbital periods of cataclysmic variables identified by the SDSS. II. Measurements for six objects, including two eclipsing systems
John Southworth, T. R. Marsh, B. T. Gaensicke +4
Continuing our work from Paper I (Southworth et al., 2006) we present medium-resolution spectroscopy and broad-band photometry of seven cataclysmic variables (CVs) discovered by th…
X-ray observations of 4 Draconis: symbiotic binary or cataclysmic triple?
Peter J. Wheatley, Koji Mukai, Domitilla de Martino
We present the first X-ray observations of the 4 Draconis system, consisting of an M3III giant with a hot ultraviolet companion. It has been claimed that the companion is itself an…
The white dwarf revealed in the intermediate polar V709 Cassiopeiae
J. M. Bonnet-Bidaud, M. Mouchet, D. de Martino +2
Results are presented from the first detailed spectroscopic observations of the recently identified intermediate polar RXJ0028.8+5917/V709 Cas. The study of the emission line radia…
A model for the optical high state light curve of AM Herculis
B. T. Gaensicke, A. Fischer, R. Silvotti +1
We present a simple quantitative model that can describe the photometric B and V band light curves of AM Herculis obtained during a high state. The double-humped shape of the V ban…
Magnetic field and unstable accretion during AM Herculis low states
J. M. Bonnet-Bidaud, M. Mouchet, N. M. Shakhovskoy +6
A study of AM Her low states in September 1990 and 1991 and June-July 1997 is reported from a coordinated campaign with observations obtained at the Haute-Provence observatory, at…