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Distance determination for RAVE stars using stellar models

ASTRONOMY & ASTROPHYSICS, (2010): null-null

Cited: 77|Views34
WOS SCOPUS

Abstract

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 ( effective temperature, surface gravity and metallicity) and (J - K-s) photometry from archival so...More

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