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- W2079259276 abstract "RAVE is a large spectroscopic survey of the Milky Way, aiming at observing up to one million stars by 2012 and at obtaining radial velocities and atmosphere parameters (see Steinmetz et al. [6], Zwitter et al. [7], Siebert et al. [5]). Despite to their medium resolution (R ∼ 7500), and the small wavelength window (8410–8795Å) RAVE spectra are suitable to perform a chemical abundance analysis. For 234,227 spectra (to date April 2011) we derived abundance estimates for up to 7 elements, which makes RAVE the largest chemical abundances database existing today. We present here the radial chemical gradients of the Milky Way by using RAVE data." @default.
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- W2079259276 date "2012-01-01" @default.
- W2079259276 modified "2023-09-25" @default.
- W2079259276 title "Investigating the Milky Way with the RAVE chemical catalog" @default.
- W2079259276 doi "https://doi.org/10.1051/epjconf/20121909005" @default.
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