Published 1991
| Published
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The tidal radii of globular clusters in M31
- Creators
-
Cohen, Judith
- Freeman, Kenneth
- Other:
- Janes, Kenneth
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
© 1991 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System.Attached Files
Published - 13-0377.pdf
Published - 1991ASPC___13__377C.pdf
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Additional details
- Eprint ID
- 96249
- Resolver ID
- CaltechAUTHORS:20190610-133424788
- Created
-
2019-06-10Created from EPrint's datestamp field
- Updated
-
2019-10-03Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 13