Distance determination for RAVE stars using stellar models

Distance determination for RAVE stars using stellar models

Show other versions (2)

(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) photometr...

Full description

Bibliographic Details
Main Authors: Breddels, M, Smith, M, Helmi, A, Bienayme, O, Binney, J, Bland-Hawthorn, J, Boeche, C, Burnett, B, Campbell, R, Freeman, K, Gibson, B, Gilmore, G, Grebel, E, Munari, U, Navarro, J, Parker, Q, Seabroke, G, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Williams, M, Wyse, R, Zwitter, T
Format: Journal article
Published: 2010

Similar Items