B, V, R Observations of the Globular Cluster System of NGC 3379

Details B, V, R Observations of the Globular Cluster System of NGC 3379 B, V, R Observations of the Globular Cluster System of NGC 3379

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.6202b&link_type=abstract

American Astronomical Society, 196th AAS Meeting, #62.02; Bulletin of the American Astronomical Society, Vol. 32, p.1284

Astronomy and Astrophysics

Astronomy

Scientific paper

NGC 3379 is a large E1 elliptical in the nearby Leo Group (d ~ 10 kpc). Because of its proximity, it was possible to reach 2 magnitudes past the expected peak of the globular cluster system luminosity function using the KPNO 4-m telescope. A field of 18 arcmin around NGC 3379 was observed in B, V and Cousins R passbands containing essentially the entire globular cluster population. Luminosity functions, colour distributions and surface density distributions of the cluster system are presented.

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