THE LARGE MAGELLANIC CLOUD INTERMEDIATE-AGE GLOBULAR CLUSTER NGC 1831

NGC 1831 is one of the largest, most populous "blue globular clusters" of the LMC. A C-M diagram to V = 21.5 shows a main sequence extending up to V = 18.5 and a well-developed giant branch. Fitting to evolutionary models leads to an age estimate of 300 million years and the giants' c...

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Veröffentlicht in:Publ. Astron. Soc. Pac.; (United States) 1984-12, Vol.96 (586), p.947-959
1. Verfasser: HODGE, PAUL W.
Format: Artikel
Sprache:eng
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Zusammenfassung:NGC 1831 is one of the largest, most populous "blue globular clusters" of the LMC. A C-M diagram to V = 21.5 shows a main sequence extending up to V = 18.5 and a well-developed giant branch. Fitting to evolutionary models leads to an age estimate of 300 million years and the giants' colors suggest that [M/H] ~ — 1.0. Spectra of three cluster stars are shown. One is for one of the "anomalous giants" and it indicates that it is probably a composite image. The spectrum of the cluster shows the dominance of the hot main sequence in the integrated light.
ISSN:0004-6280
1538-3873
DOI:10.1086/131458