CCD Photometry of the Globular Cluster NGC 4372

Details CCD Photometry of the Globular Cluster NGC 4372 CCD Photometry of the Globular Cluster NGC 4372

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994jass...11..147y&link_type=abstract

Journal of Astronomy and Space Science, vol. 11, no. 2, p. 147-153.

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a deep (B, V) color-magnitude diagram (CMD) of the Galactic globular cluster NGC 4372. According to the recent inside-out picture of Galaxy formation, this cluster is predicted to be one of the oldest globular clusters in the Galaxy. Our CMD shows a well defined main-sequence extending +/- 2 magnitudes below the turnoff. Despite the uncertainty that stems from, the small sample size of bright stars, comparison with the Revised Yale Isochrones suggests in our Galaxy.

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