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The tidal radii of globular clusters in M31

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. 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/115699DOIArticle
http://adsabs.harvard.edu/abs/1991AJ....101..483CADSArticle
ORCID:
AuthorORCID
Cohen, J. G.0000-0002-8039-4673
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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Caltech Recycling CenterUNSPECIFIED
Issue or Number:2
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
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Deposited By: George Porter
Deposited On:04 Jun 2019 20:31
Last Modified:03 Oct 2019 21:19

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