The tidal radii of globular clusters in M31

Details The tidal radii of globular clusters in M31 The tidal radii of globular clusters in M31

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101..483c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, Feb. 1991, p. 483-489. Research supported by California Institute of Technology

Astronomy and Astrophysics

Astronomy

25

Andromeda Galaxy, Globular Clusters, Eccentricity, Error Analysis, Spatial Distribution

Scientific paper

Tidal radii have been determined 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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