Statistical method for distance determination of a stellar group
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 frequency function of the apparent magnitudes, so as to correct for observational incompleteness at the faint end. The problem reduces to the solution of a highly transcendental equation for a given apparent magnitude parameter alpha . Computational algorithm of the method is illustrated and the numerical solutions of the basic equation are given for some values of alpha .
- Publication:
-
Astronomische Nachrichten
- Pub Date:
- 2003
- DOI:
- 10.1002/asna.200310086
- Bibcode:
- 2003AN....324..238S
- Keywords:
-
- stars: distances;
- stars: fundamental parameters;
- stars: statistics;
- Galaxy: stellar groups