Why Are The Secondary Stars in Polars So Normal?

Details Why Are The Secondary Stars in Polars So Normal? Why Are The Secondary Stars in Polars So Normal?

2005-09-15

arxiv.org/abs/astro-ph/0509457v1

Astrophys.J.632:L123-L126,2005

Astronomy and Astrophysics

Astrophysics

16 pages, 2 figures

Scientific paper

10.1086/498067

We have used NIRSPEC on Keck II to obtain $K$-band spectroscopy of several magnetic cataclysmic variables. These data reveal that the secondary stars in these binary systems have spectra that are consistent with normal, late-type dwarfs in both their atomic and molecular line strengths, as well as in the slopes of their continuua. This result is in stark contrast to the infrared spectra of their non-magnetic cousins, nearly all of which show peculiar abundances, especially of CNO species and their isotopes. It appears that the evolutionary path taken by the secondary stars in magnetic systems differs from that for the non-magnetic systems. We discuss the implications of this result.

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