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Middle- and Far-Ultraviolet Observations of Hot White Dwarfs

Published online by Cambridge University Press:  12 April 2016

S. B. Parsons ,
J. D. Wray  and
K. G. Henize
S. B. Parsons
Affiliation:
Department of Astronomy, University of Texas at Austin
J. D. Wray
Affiliation:
Department of Astronomy, University of Texas at Austin
K. G. Henize
Affiliation:
Department of Astronomy, University of Texas at Austin

Extract

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Several hot subluminous stars were first recognized as such from low-resolution spectra obtained with the ultraviolet objective-prism survey from Skylab, Experiment S-019. About 9 percent of the sky was photographed, 3 percent with unwidened spectra. Two hot subdwarf stars have been reported previously, HDE 283048 (Laget et al. 1978) and the companion to HR 3080 (Parsons et al. 1976a). Papers on two other subdwarfs are in preparation. One previously unrecognized white dwarf star was found, HD 149499 B, and new observations (Wray, Parsons and Henize 1979) show it to be probably the hottest white dwarf known.

Type
Colloquium Session II
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 109 - 113
Copyright
Copyright © The University of Rochester 1979

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