Analysis of MV Lyrae in a low state

Details Analysis of MV Lyrae in a low state Analysis of MV Lyrae in a low state

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348..266l&link_type=abstract

Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE ASP Conference Series, Vol. 348, Proceedings of the Confe

Astronomy and Astrophysics

Astrophysics

Scientific paper

A recent analysis by Hoard et al. of FUSE and optical spectra of the nova-like cataclysmic variable MV Lyrae derived a system model and associated synthetic spectrum which accurately fit the observed spectra. Yet that model, with an orbital inclination from the literature of i=12°, produced a synthetic light curve with an amplitude appreciably larger than observed.
We show that optimized light curve fitting, based on our spectrum analysis model, determines an orbital inclination of 7°.

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