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Published 1990 | Version Published
Book Section - Chapter Open

Structural Parameters for Globular Clusters in M 31

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Abstract

After a review of existing data on structural parameters for globular clusters, we present new measurements of tidal radii for 30 globular clusters in M 31. These measurements are consistent with the globular clusters in M 31 having the same mean M/L ratio as those in the Galaxy.

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© 1990 L. Davis Press. Provided by the NASA Astrophysics Data System.

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Published - 1990ccd2_conf__167C.pdf

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1990ccd2_conf__167C.pdf

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96248
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CaltechAUTHORS:20190610-132642801

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http://adsabs.harvard.edu/abs/1990ccd2.conf..167C (URL)

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2019-06-10
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2019-10-03
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Contributions of the VanVleck Observatory
Series Volume or Issue Number
10