Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes
Date
2006Author
Karataş, Yüksel
Güver, Tolga
Karaali, Salih
Bilir, Selçuk
Ak, Serap
Metadata
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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.
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