Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way. We use the subsample of spectra with spectroscopically determined values of stellar parameters to determine the distances to these stars. The list currently contains 235,064 high quality spectra which show no peculiari...
Huvudupphovsmän: | Zwitter, T, vc, G, Breddels, M, Smith, M, Helmi, A, Munari, U, Bienaymé, O, Binney, J, Bland-Hawthorn, J, Boeche, C, Brown, A, Campbell, R, Freeman, K, Fulbright, J, Gibson, B, Gilmore, G, Grebel, E, Navarro, J, Parker, Q, Seabroke, G, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Williams, M |
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Materialtyp: | Journal article |
Språk: | English |
Publicerad: |
2010
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Liknande verk
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Distance determination for RAVE stars using stellar models: II. Most likely values assuming a standard stellar evolution scenario
av: Zwitter, T, et al.
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Distance determination for RAVE stars using stellar models
av: Breddels, M, et al.
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models III. The nature of the RAVE survey and Milky Way chemistry
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