Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes
- 16 January 2006
- journal article
- Published by Wiley in Astronomische Nachrichten
- Vol. 327 (1) , 72-81
- https://doi.org/10.1002/asna.200510480
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This publication has 28 references indexed in Scilit:
- The thick disc component of the Galaxy from near infrared colour–magnitude diagramsAstronomy & Astrophysics, 2005
- Comprehensive Analysis of RGU Photometry in the Direction to M5Publications of the Astronomical Society of Australia, 2004
- The ROTSE‐III Robotic Telescope SystemPublications of the Astronomical Society of the Pacific, 2003
- Catalogue of [Fe/H] determinations for FGK stars: 2001 editionAstronomy & Astrophysics, 2001
- Stellar Population Studies with the SDSS. I. The Vertical Distribution of Stars in the Milky WayThe Astrophysical Journal, 2001
- Metal–poor turnoff and subgiant field stars in the GalaxyAstronomy and Astrophysics Supplement Series, 1998
- Kinematics of metal-poor stars in the galaxyThe Astrophysical Journal Supplement Series, 1995
- A survey of proper-motion stars. X - The early evolution of the Galaxy's haloThe Astronomical Journal, 1990
- Comparisons of a standard galaxy model with stellar observations in five fieldsThe Astrophysical Journal Supplement Series, 1984
- New light on faint stars – III. Galactic structure towards the South Pole and the Galactic thick discMonthly Notices of the Royal Astronomical Society, 1983