Low Mass Stars in an Outer Field in NGC 6397

Details Low Mass Stars in an Outer Field in NGC 6397 Low Mass Stars in an Outer Field in NGC 6397

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pasp..108..682m&link_type=abstract

Publications of the Astronomical Society of the Pacific, v.108, p.682

Astronomy and Astrophysics

Astronomy

8

Globular Clusters: Individual: Ngc 6397, Stars: Low-Mass

Scientific paper

We have imagined a field 10' from the center of the globular cluster NGC 6397 in the visible and I bands with WFPC-2 on the HST. AT a level which is severely limited by counting statistics in the small area so far studied, this field is richer in dwarfs with I > 21.5 than the 4.6' radius parallel field discussed by Paresce and colleagues. This indicates that the dynamical process of mass segregation is occurring in the cluster. (SECTION: Stellar Clusters and Associations)

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