Cohen, Judith and Freeman, Kenneth (1991) The tidal radii of globular clusters in M31. In: The formation and evolution of star clusters. Astronomical Society of the Pacific Conference Series. No.13. Astronomical Society of the Pacific , San Francisco, CA, pp. 377-380. ISBN 9780937707326. https://resolver.caltech.edu/CaltechAUTHORS:20190610-133424788
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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: | © 1991 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System. | |||||||||
| Series Name: | Astronomical Society of the Pacific Conference Series | |||||||||
| Issue or Number: | 13 | |||||||||
| Record Number: | CaltechAUTHORS:20190610-133424788 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190610-133424788 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 96249 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 10 Jun 2019 20:45 | |||||||||
| Last Modified: | 03 Oct 2019 21:20 |
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