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Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
- Volume 5, Issue 31 - article #6
- T. Zwitter (1 and 2), G. Matijeviv{c) (1), M. A. Breddels (3), M. C. Smith (3, 4), A. Helmi (3), U. Munari (5), O. Bienaym'{e) (6), J. Binney (7), J. Bland-Hawthorn (8), C. Boeche (9), A. G. A. Brown (10), R. Campbell (11), K. C. Freeman (12), J. Fulbright (13), B. Gibson (14), G. Gilmore (15), E. K. Grebel (16), J. F. Navarro (17), Q. A. Parker (18), G. M. Seabroke (19), A. Siebert (6), A. Siviero (5, 9), M. Steinmetz (9), F. G. Watson (20), M. Williams (9), R. F. G. Wyse (13) ((1) University of Ljubljana, Faculty of Mathematics, Physics, Ljubljana, Slovenia} (2) Center of excellence SPACE-SI, Ljubljana, Slovenia, (3) Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands, (4) Kavli Institute for Astronomy, Astrophysics, Peking University, Beijing, China, (5) INAF Astronomical Observatory of Padova, et al. (36 additional authors not shown)
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4411 [pdf, ps, other]

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