Density profiles and luminosity functions of the globular clusters M3 and M92

Details Density profiles and luminosity functions of the globular clusters M3 and M92 Density profiles and luminosity functions of the globular clusters M3 and M92

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992an....313...45s&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 313, no. 1, 1992, p. 45-52. Research supported by Cambridge University Institut

Astronomy and Astrophysics

Astronomy

7

Astrometry, Density Distribution, Globular Clusters, Star Distribution, Stellar Luminosity, Photographic Plates, Separation

Scientific paper

Tautenburg Schmidt plates with the globular clusters M3 and M92 were measured on the APM facility in Cambridge, mainly for astrometric purposes. The data were used to derive the radial density profiles and the luminosity functions of these clusters. There is a good agreement of the present results with earlier ones derived by other authors. In both clusters effects of mass segregation are observed.

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