Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes

Preprint

13 August 2005

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0508307

Abstract

We present a procedure which separates field dwarfs and field giants by their 2MASS and V apparent magnitudes. The procedure is based on the spectroscopically selected standards, hence it is confident. We applied this procedure 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 appeared recently in the literature.

Keywords

GALACTIC MODEL PARAMETERS
SEPARATED FROM FIELD
APPARENT MAGNITUDES
GIANTS SEPARATED
FIELD GIANTS
FIELD DWARFS
2MASS

All Related Versions

Version 1, 2005-08-13, ArXiv
Published version: Astronomische Nachrichten, 327 (1), 72.

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