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Bilir S., Karaali S., Güver T., Karataş Y., Ak S.
ASTRONOMISCHE NACHRICHTEN, vol.327, no.1, pp.72-81, 2006 (SCI-Expanded)
Article / Article
Science Citation Index Expanded (SCI-EXPANDED), Scopus
Galaxy : structure, Galaxy : fundamental parameters, stars : giants, STELLAR LUMINOSITY FUNCTION, PROPER-MOTION STARS, RGU PHOTOMETRY, GALAXY MODELS, OLD STARS, KINEMATICS, POPULATION, ABUNDANCE, COUNTS, HALO
Istanbul University Affiliated:
We present a method which separates field dwarfs and field giants by their 2MASS and V apparent magnitudes. This method is based on spectroscopically selected standards and is hence reliable. We applied it to stars in two fields, SA 54 and SA 82, and we estimated a full set of Galactic model parameters for giants including their total local space density. Our results are in agreement with the ones given in the recent literature.