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Searches for Binary Stars in Globular Clusters

Published online by Cambridge University Press:  25 May 2016

C. Pryor
Affiliation:
Rutgers, the State University of New Jersey, Dept. of Physics & Astronomy, P.O. Box 849, Piscataway, NJ 08855-0849 USA
J.M. Fletcher
Affiliation:
Dominion Astrophysical Observatory, HIA/NRC
J.E. Hesser
Affiliation:
Dominion Astrophysical Observatory, HIA/NRC
R.D. McClure
Affiliation:
Dominion Astrophysical Observatory, HIA/NRC
P.B. Stetson
Affiliation:
Dominion Astrophysical Observatory, HIA/NRC
H.B. Richer
Affiliation:
Univ. of British Columbia, Dept. of Geophysics & Astronomy
G.G. Fahlman
Affiliation:
Univ. of British Columbia, Dept. of Geophysics & Astronomy
R.A. Ibata
Affiliation:
Univ. of British Columbia, Dept. of Geophysics & Astronomy
N.C. Ivanans
Affiliation:
Univ. of British Columbia, Dept. of Geophysics & Astronomy
G. Mandushev
Affiliation:
Univ. of British Columbia, Dept. of Geophysics & Astronomy
R.A. Bell
Affiliation:
Univ. of Maryland, Dept. of Astronomy
M. Bolte
Affiliation:
Univ. of California, Lick Observatory
H.E. Bond
Affiliation:
Space Telescope Science Institute
W.E. Harris
Affiliation:
McMaster Univ., Dept. of Physics & Astronomy
D.A. Vandenberg
Affiliation:
Univ. of Victoria, Dept. of Physics & Astronomy
M.A. Wood
Affiliation:
Florida Institute of Technology, Dept. of Physics & Space Science

Extract

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Primordial binaries in globular clusters are important both because their properties are an integral part of the description of the stellar population and because they can strongly influence the dynamical evolution of the cluster (see Hut, this volume).

Type
August 25: X Ray and Compact Objects in Globular Clusters
Copyright
Copyright © Kluwer 1996 

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