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The stellar content and distance of UGC 4483

✍ Scribed by A. E. Dolphin; L. Makarova; I. D. Karachentsev; V. E. Karachentseva; D. Geisler; E. K. Grebel; P. Guhathakurta; P. W. Hodge; A. Sarajedini; P. Seitzer


Publisher
John Wiley and Sons
Year
2001
Tongue
English
Weight
346 KB
Volume
324
Category
Article
ISSN
0035-8711

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## Abstract In this paper, we developed statistical method for distance determination of a stellar group. The method depends on the assumption that, the stars scatter around a mean magnitude in a Gaussian distribution. The mean apparent magnitude of the stars is then expressed in terms of the frequ