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

Harrison T. E.; Howell S. B.; Johnson J. J.; Osborne H. L.; Homeier D.

Vol. 20 No. 1 (2004), Contributions

Vol. 20 No. 1 (2004)

Contributions

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

Harrison T. E.⁺⁻
Howell S. B.⁺⁻
Johnson J. J.⁺⁻
Osborne H. L.⁺⁻
Homeier D.⁺⁻

Harrison T. E.

New Mexico State University, Box 30001/MSC4500, Las Cruces, NM 88003 USA

Howell S. B.

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Johnson J. J.

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Osborne H. L.

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Homeier D.

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Keywords

Novae
Cataclysmic variables

How to Cite

Peculiar Abundances in CV Secondary Stars: Revising their Evolutionary History?. (2004). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 20(1), 249-249. https://astronomia.unam.mx/journals/rmxac/article/view/2004rmxac..20..249h

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Abstract

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

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