Published 1990
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Structural Parameters for Globular Clusters in M 31
- Creators
-
Cohen, Judith G.
Chicago
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Abstract
After a review of existing data on structural parameters for globular clusters, we present new measurements of tidal radii for 30 globular clusters in M 31. These measurements are consistent with the globular clusters in M 31 having the same mean M/L ratio as those in the Galaxy.
Additional Information
© 1990 L. Davis Press. Provided by the NASA Astrophysics Data System.Attached Files
Published - 1990ccd2_conf__167C.pdf
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1990ccd2_conf__167C.pdf
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Additional details
- Eprint ID
- 96248
- Resolver ID
- CaltechAUTHORS:20190610-132642801
- Created
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2019-06-10Created from EPrint's datestamp field
- Updated
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2019-10-03Created from EPrint's last_modified field
- Series Name
- Contributions of the VanVleck Observatory
- Series Volume or Issue Number
- 10