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A spectroscopic determination of the mass distribution of DA white dwarfs

Bergeron, P., Saffer, Rex A., Liebert, James·1992·The Astrophysical Journal

Abstract

Attention is given to the mass distribution for a sample of 129 DA white dwarfs based on fitting hydrogen line profiles to the predictions of stellar atmosphere models. The atmospheric parameters determined from spectroscopy are shown to be of improved accuracy over those obtained with other techniques. The spectroscopic masses are in good agreement with those inferred from gravitational redshift measurements. The masses obtained for the stars in the Hyades cluster are found to be measurably higher than those obtained from trigonometric parallaxes, although the observed scatter is greatly reduced in the spectroscopic analysis. The observed mass distribution exhibits a narrow peak, but broad and flat tails extend to large and small masses. The mean mass of the distribution is somewhat lower - near 0.56 solar mass - than found in the best previous analyses. The consequences of these results for earlier phases of stellar evolution are discussed.

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Metadata

Authors
Bergeron, P., Saffer, R. A., & Liebert, J.
Venue
The Astrophysical Journal
Published
1992-07
Volume
394
Pages
228
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2996098872
Cited by
559
References
0
FWCI
15.07
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A spectroscopic determination of the mass distribution of DA white dwarfs. https://app.cochat.ai/papers/10.1086/171575
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Bergeron, P., Saffer, R. A., & Liebert, J. (1992). A spectroscopic determination of the mass distribution of DA white dwarfs. The Astrophysical Journal. https://doi.org/10.1086/171575

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