An IR study of the eclipsing dwarf nova IP Pegasi

Details An IR study of the eclipsing dwarf nova IP Pegasi An IR study of the eclipsing dwarf nova IP Pegasi

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330..369r&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

Scientific paper

We report the analysis of JHK light curves of the eclipsing dwarf nova IP Pegasi obtained with the 4.2m WHT Telescope at La Palma on 1996 October 26-29 while the system was in quiescence. We model the observed ellipsoidal modulation to estimate the binary parameters and we apply eclipse mapping techniques to map the surface brightness distributions of the accretion disc.

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