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Constraints on the age and evolution of the Galaxy from the white dwarf luminosity function

Wood, M. A.·1992·The Astrophysical Journal

Abstract

The white dwarf disk luminosity function is explored using observational results of Liebert et al. (1988, 1989) as a template for comparison, and the cooling curves of Wood (1990, 1991) as the input basis functions for the integration. The star formation rate over the history of the Galaxy is found to be constant to within an order of magnitude, and the disk age lies in the range 6-13.5 Gyr, where roughly 40 percent of the uncertainty is due to the observational uncertainties. Using the best current estimates as inputs to the integration, the disk ages range from 7.5 to 11 Gyr, i.e., they are substantially younger than most estimates for the halo globular clusters but in reasonable agreement with those for the disk globular clusters and open clusters. The ages of these differing populations, taken together, are consistent with the pressure-supported collapse models of early spiral Galactic evolution.

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Metadata

Authors
Wood, M. A.
Venue
The Astrophysical Journal
Published
1992-02
Volume
386
Pages
539
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2051825590
Cited by
270
References
0
FWCI
16.38
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Constraints on the age and evolution of the Galaxy from the white dwarf luminosity function. https://app.cochat.ai/papers/10.1086/171038
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Wood, M. A. (1992). Constraints on the age and evolution of the Galaxy from the white dwarf luminosity function. The Astrophysical Journal. https://doi.org/10.1086/171038

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