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Published 1991 | Version Published
Book Section - Chapter Open

The tidal radii of globular clusters in M31

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Abstract

We have determined tidal radii for 30 globular clusters in the halo of M31 from deep direct images. Although the uncertainty of each individual measurement is large, in the mean the tidal radii suggest that the M31 globular clusters have orbital eccentricities and mass-to-light ratios that are very similar to those of Galactic globular clusters.

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© 1991 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System.

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Published - 13-0377.pdf

Published - 1991ASPC___13__377C.pdf

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96249
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CaltechAUTHORS:20190610-133424788

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http://adsabs.harvard.edu/abs/1991ASPC...13..377C (URL)

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2019-06-10
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2019-10-03
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Series Name
Astronomical Society of the Pacific Conference Series
Series Volume or Issue Number
13