Photometric evidence of superhumps in XTE J1118+48 approaching quiescence

Details Photometric evidence of superhumps in XTE J1118+48 approaching quiescence Photometric evidence of superhumps in XTE J1118+48 approaching quiescence

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..473c&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

Ellipsoidal lightcurves of XTE J1118+48 during its decline to quiescence
are strongly contaminated with a superhump wave. A PDM period analysis
yields Psh = 0.17049(1) d i.e. 0.3% longer than the orbital
period. This implies a disc precession period Pprec ~52 d and
q ~0.03.

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