Abstract
We report on the analysis of optical and FUV spectra of a sample of DAO white dwarfs. Optical spectra obtained at Kitt Peak were used to determine their temperature and gravity and compared with results from Lyman series observations made by the FUSE satellite. Significant differences were found between the Balmer and Lyman line techniques. Most of the objects in the sample were found to consist of low gravity, high temperature objects and hence have low mass, with one DAO already known to be the result of common envelope evolution. Overall the results from the DAO stars can now be compared with the larger population of DA white dwarfs.
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© 2003 Springer Science+Business Media Dordrecht
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Good, S.A. et al. (2003). Spectroscopic Determination of Mass for a Sample of DAO White Dwarfs. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_41
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DOI: https://doi.org/10.1007/978-94-010-0215-8_41
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-1364-5
Online ISBN: 978-94-010-0215-8
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