An eclipse of the X-ray flux from the dwarf nova OY Carinae in quiescence

Details An eclipse of the X-ray flux from the dwarf nova OY Carinae in quiescence An eclipse of the X-ray flux from the dwarf nova OY Carinae in quiescence

1999-03-03

arxiv.org/abs/astro-ph/9903058v1

Mon.Not.Roy.Astron.Soc. 307 (1999) 413-419

Astronomy and Astrophysics

Astrophysics

7 pages, 6 figures, uses psfig.sty and mn.sty, accepted for publication in Monthly Notices of the Royal Astronomical Society

Scientific paper

10.1046/j.1365-8711.1999.02601.x

We present a phase-resolved ROSAT HRI X-ray light curve of the dwarf nova OY
Car in quiescence. The X-ray flux is eclipsed at the same time as the optical
eclipse of the primary, and the region of X -ray emission is comparable in size
to the white dwarf. We use subsequent optical observations to update the
orbital ephemeris of the system.

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