Published February 1991
| Published
Journal Article
Open
The tidal radii of globular clusters in M31
- Creators
-
Cohen, J. G.
- Freeman, K. C.
Chicago
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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.
Additional Information
© American Astronomical Society Provided by the NASA Astrophysics Data System. Received 11 July 1990; revised 16 October 1990. J.G.C. and K.C.F. are grateful to the Aspen Center for Physics for hospitality while the final draft of this paper was written. J.G.C. is grateful to the Caltech Recycling Center for financial support.Attached Files
Published - 1991AJ____101__483C.pdf
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1991AJ____101__483C.pdf
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Additional details
- Eprint ID
- 96077
- Resolver ID
- CaltechAUTHORS:20190603-153224172
- Caltech Recycling Center
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2019-06-04Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field