- Abstract:
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(Abridged) Aims:We develop a method for deriving distances from spectroscopic data and obtaining full 6D phase-space coordinates for the RAVE survey's second data release. Methods: We used stellar models combined with atmospheric properties from RAVE (Teff, logg and [Fe/H]) and (J-Ks) photometry from archival sources to derive absolute magnitudes. We are able to derive the full 6D phase-space coordinates for a large sample of RAVE stars. This method is tested with artificial data, Hipparcos t...
Expand abstract - Publication date:
- 2010-03-03
- URN:
-
uuid:8fea2636-dea3-4e96-b42c-9164ee5114ca
- Source identifiers:
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167427
- Local pid:
- pubs:167427
- Keywords:
- Copyright date:
- 2010
- Notes:
-
17 pages, 18 figures, data and future updates available at
http://www.astro.rug.nl/~rave, accepted for publication in AandA
Journal article
Distance determination for RAVE stars using stellar models
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