Globular Clusters in the Magellanic Clouds.I:BV CCD-Photometry for 11 Clusters

Details Globular Clusters in the Magellanic Clouds.I:BV CCD-Photometry for 11 Clusters Globular Clusters in the Magellanic Clouds.I:BV CCD-Photometry for 11 Clusters

1994-09-29

arxiv.org/abs/astro-ph/9409084v1

Astronomy and Astrophysics

Astrophysics

62 pages, 37 figures and tables 6 to 16 available on request, uuencoded compressed postscript file with tables 1-5 and 17-18 i

Scientific paper

We present BV CCD-data for 11 intermediate-age LMC clusters; the main conclusions are: 1. in the (V_to, V_cl,m) and (V-to, (V_to-V_cl,m)) planes the models yield a good overall description of the data; 2. with the current sample, it is impossible to firmly choose between "classical" and "overshooting" models; 3. the separation in colour between the MS band and the Red He-burning Clump is smaller than predicted by theoretical tracks; 4. the existence of the so-called "RGB phase-transition (Renzini and Buzzoni 1986) seems to be confirmed.

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