Heavy element abundances predicted by radiative support theory in the atmospheres of hot white dwarfs

Author:

Chayer P.,Fontaine G.,Wesemael F.

Publisher

Springer Berlin Heidelberg

Reference12 articles.

1. Bergeron, P., Wesemael, F., Michaud, G., and Fontaine, G. 1988,Ap. J., in press.

2. Bruhweiler, F.C. 1985, Bull. Amen. Astorn. Soc., 17, 559.

3. Bruhweiler, F.C., and Kondo, Y. 1981, Ap. J. (Letters), 248, L123.

4. Bruhweiler, F.C., and Kondo, Y. 1983, Ap. J., 269, 657.

5. Chayer, P., Fontaine, G., Wesemael, F. and Michaud, G. 1987, in IAU Colloquium No. 95, The Second Conference on Feint Blue Stars, A. G. D. Philip, D. S. Hayes and J. Liebert, eds., L. Davis Press, Schenectady, p. 653.

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1. Stratified NLTE Model Atmospheres for Hot Stars;Symposium - International Astronomical Union;2003

2. Far and Extreme Ultraviolet Spectroscopy of Hot White Dwarf Stars: A Laboratory for Element Diffusion;Astrophysics and Space Science Library;1994

3. Diffusion of Heavy Elements in White Dwarfs with Radiative Forces and Mass Loss;White Dwarfs: Advances in Observation and Theory;1993

4. Early White Dwarf Results from EUVE;White Dwarfs: Advances in Observation and Theory;1993

5. Stratification in White Dwarf Atmospheres;Symposium - International Astronomical Union;1991

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