Cohen, J. G. and Freeman, K. C. (1991) The tidal radii of globular clusters in M31. Astronomical Journal, 101 (2). pp. 483-489. ISSN 0004-6256. doi:10.1086/115699. https://resolver.caltech.edu/CaltechAUTHORS:20190603-153224172
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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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| 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. | |||||||||
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| Issue or Number: | 2 | |||||||||
| DOI: | 10.1086/115699 | |||||||||
| Record Number: | CaltechAUTHORS:20190603-153224172 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190603-153224172 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 96077 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 04 Jun 2019 20:31 | |||||||||
| Last Modified: | 16 Nov 2021 17:17 |
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