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The White Dwarf Cooling Sequence of the Globular Cluster Messier 4

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Hansen, Brad M. S., Brewer, James, Fahlman, Greg G., Gibson, Brad K., Ibata, Rodrigo, Limongi, Marco, Rich, R. Michael, Richer, Harvey B., Shara, Michael M., Stetson, Peter B.·2002·The Astrophysical Journal

Abstract

We present the white dwarf sequence of the globular cluster M4, based on a 123 orbit Hubble Space Telescope exposure, with a limiting magnitude of V ~ 30 and I ~ 28. The white dwarf luminosity function rises sharply for I > 25.5, consistent with the behavior expected for a burst population. The white dwarfs of M4 extend to approximately 2.5 mag fainter than the peak of the local Galactic disk white dwarf luminosity function. This demonstrates a clear and significant age difference between the Galactic disk and the halo globular cluster M4. Using the same standard white dwarf models to fit each luminosity function yields ages of 7.3 ± 1.5 Gyr for the disk and 12.7 ± 0.7 Gyr for M4 (2 σ statistical errors).

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Metadata

Authors
Hansen, B. M. S., Brewer, J., Fahlman, G. G., Gibson, B. K., Ibata, R., Limongi, M., Rich, R. M., Richer, H. B., Shara, M. M., & Stetson, P. B.
Venue
The Astrophysical Journal
Published
2002-08-01
Volume
574
Issue
2
Pages
L155-L158
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2107693062
Cited by
249
References
0
FWCI
14.81
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The White Dwarf Cooling Sequence of the Globular Cluster Messier 4. https://app.cochat.ai/papers/10.1086/342528
The paper
Hansen, B. M. S., Brewer, J., Fahlman, G. G., Gibson, B. K., Ibata, R., Limongi, M., Rich, R. M., Richer, H. B., Shara, M. M., & Stetson, P. B. (2002). The White Dwarf Cooling Sequence of the Globular Cluster Messier 4. The Astrophysical Journal. https://doi.org/10.1086/342528

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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