The structure of the accretion disk rim in supersoft X-ray sources.

Details The structure of the accretion disk rim in supersoft X-ray sources. The structure of the accretion disk rim in supersoft X-ray sources.

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...321..245m&link_type=abstract

Astronomy and Astrophysics, v.321, p.245-253

Astronomy and Astrophysics

Astrophysics

39

Accretion Disks, Binaries: Eclipsing, Stars: Individual: Cal 87, Rx J0019.8+2156, Rx J0513.9-6951, X-Rays: Stars

Scientific paper

Supersoft X-ray sources are characterized by the radiation of a white dwarf with a temperature of some 10^5^K. The compact star is surrounded by an irradiated accretion disk which provides the high optical luminosity. For CAL 87 (Schandl et al. 1996LNP96.472...53S, 1996A&A...318...73S) it could be shown, that this disk has an elevated rim at the outer edge. The impact of the accretion stream from the companion on the disk is important for the rim structure. More optical observations have recently become available for supersoft sources. Detailed features became known, as short-time variations of the shape of the orbital light curve of RX J0019 (Will & Barwig 1996), the long-term variations of RX J0019 (Greiner & Wenzel 1995A&A...294L...5G) and the changes of RX J0513 between a high and a low state (Alcock et al. 1996MNRAS.280L..49A). We use our simulation of the orbital light curves (developed for CAL 87) to analyse the disk rim structure of these two other sources in comparison with the observations. We find that a high rim gives good agreement and allows to explain the observations. For the modelling of the high state of RX J0513 the irradiation of disk and secondary by an extended white dwarf is included. The consistent appearance of a high rim feature raises interesting dynamical problems for the stream disk interaction.

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