Deep CCD Photometry of Stars in the Globular Cluster M3

Details Deep CCD Photometry of Stars in the Globular Cluster M3 Deep CCD Photometry of Stars in the Globular Cluster M3

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169...15p&link_type=abstract

Astrophysics and Space Science, Volume 169, Issue 1-2, pp. 15-18

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Preliminary results on new CCD photometry inV andB bands of approximately 5000 stars in four overlapping fields in the globular cluster M3 are presented. The colour-magnitude diagram shows a very well-defined sequence with a small scatter, going fainter than previously published work on this cluster. The turn-off point found atV=19.1±0.2 mag and (B-V)=0.445±0.01, is slightly redder than those obtained in previous studies.

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