The Detection of 13CO and Other Apparent Abundance Anomalies in the Secondary Stars of Long-Period Cataclysmic Variables

Details The Detection of 13CO and Other Apparent Abundance Anomalies in the Secondary Stars of Long-Period Cataclysmic Variables The Detection of 13CO and Other Apparent Abundance Anomalies in the Secondary Stars of Long-Period Cataclysmic Variables

2004-02-19

arxiv.org/abs/astro-ph/0402470v1

Astronomy and Astrophysics

Astrophysics

43 pages, 20 figures

Scientific paper

10.1086/420706

We present moderate resolution (R > 1,800) infrared K-band spectra of twelve long-period (Porb > 6 hr) cataclysmic variables. We detect absorption lines from the photospheres of the secondary stars in every system, even though two of the m were undergoing outubrsts. We have attempted to assign spectral types to each of the secondary stars, and these classifications are generally consistent with previous determinations/estimates. We find evidence for abundance anomalies that include enhancements and/or deficits for all of the species commonly found in the K-band spectra of G- and K-type dwarfs. There is, however, only one common abundance anomaly: extremely weak CO features. Only two of the twelve objects appeared to have normal levels of CO absorption. We interpret this as evidence for low carbon abundances. In addition, we detect 13CO absorption in four of the twelve objects. Depleted levels of 12C and enhanced levels of 13C indicate that material that has been processed in the CNO cycle is finding its way into the photospheres of CV secondary stars. In systems with luminous accretion disks, we find that the spectrum of the secondary star is contaminated by a source that flattens (reddens) the continuum. While free-free or classical accretion disk spectra are flatter than the blackbody-like spectra of G and K dwarfs, removal of such contamination from the K-band data results in spectra in which the absorption features become too strong to be consistent with those of G and K dwarfs.

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