## 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
β¦ LIBER β¦
Computational developments for distance determination of stellar groups
β Scribed by M. A. Sharaf; A. M. Sendi
- Book ID
- 107582844
- Publisher
- Springer-Verlag
- Year
- 2010
- Tongue
- English
- Weight
- 214 KB
- Volume
- 31
- Category
- Article
- ISSN
- 0250-6335
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