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ROSAT Studies of the Composition and Structure of DA White Dwarf Atmospheres

Published online by Cambridge University Press:  07 August 2017

C.J. Diamond
Affiliation:
1School of Physics and Space Research, University of Birmingham, UK
M.A. Barstow
Affiliation:
2Dept. of Physics and Astronomy, Univeristy of Leicester, UK
A.E. Sansom
Affiliation:
2Dept. of Physics and Astronomy, Univeristy of Leicester, UK
M.C. Marsh
Affiliation:
2Dept. of Physics and Astronomy, Univeristy of Leicester, UK
S.R. Rosen
Affiliation:
2Dept. of Physics and Astronomy, Univeristy of Leicester, UK
T.A. Fleming
Affiliation:
3Max-Planck-Institut Für Extraterrestrische Physik, Garching, GER
D. Koester
Affiliation:
4Dept. of Physics and Astronomy, Louisiana State University, Baton Rouge, USA
D.S. Finley
Affiliation:
5Center for EUV Astrophysics, University of California, Berkeley, USA
J.B. Holberg
Affiliation:
6Lunar and Planetary Laboratory, University of Arizona, Tucson, USA
K. Kidder
Affiliation:
6Lunar and Planetary Laboratory, University of Arizona, Tucson, USA

Extract

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We have made a detailed study of a sample of 28 hot DA white dwarfs detected in the ROSAT EUV and soft X-ray all-sky-survey.

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Copyright
Copyright © Kluwer 1993 

References

1. Vennes, S., Thejll, P., & Shipman, H.L., in White Dwarfs, ed. Wegner, G., Springer-Verlag, 176.Google Scholar
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3. Wilkinson, E., Cash, W. & Green, J.C., 1992, Ap.J , submitted.Google Scholar
4. Chayer, et al., 1989, in ‘ White Dwarfs ’, ed. Wegner, G., Springer-Verlag, 176.Google Scholar