Peculiar Abundances in CV Secondary Stars: Revising their Evolutionary History?

Details Peculiar Abundances in CV Secondary Stars: Revising their Evolutionary History? Peculiar Abundances in CV Secondary Stars: Revising their Evolutionary History?

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..249h&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

2

Novae, Cataclysmic Variables

Scientific paper

We have recently completed an infrared (K-band) spectroscopic survey of
two dozen cataclysmic variables. The systems range in orbital period
from P [orb] = 1.35 hr (EF Eri), to P [orb] = 11.0 hr (V442 Cen). We
detect the secondary star in every system.

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