Limits on the orbital eccentricities of globular clusters

Details Limits on the orbital eccentricities of globular clusters Limits on the orbital eccentricities of globular clusters

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..48..191h&link_type=abstract

Astrophysics and Space Science, vol. 48, no. 1, May 1977, p. 191-197.

Astronomy and Astrophysics

Astrophysics

8

Celestial Mechanics, Eccentricity, Globular Clusters, Milky Way Galaxy, Orbital Mechanics, Astronomical Models, Orbital Elements

Scientific paper

By use of an inverse-square mass-model for the Galaxy, the range in
eccentricities for the orbits of 57 globular clusters is computed. On
the assumption that all clusters have the same apogalacticon distance,
various values of this distance are considered. It is found that low
eccentricities are possible for small apogalacticon distances

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