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COELHO, P; BARBUY, B; MELENDEZ, J; SCHIAVON, R. P; CASTILHO, B. V
Astronomy and astrophysics (Berlin), 11/2005, Letnik: 443, Številka: 2Journal Article
Libraries of stellar spectra are fundamental tools for the study of stellar populations, and both empirical and synthetic libraries have been used for this purpose. In this paper, a new library of high resolution synthetic spectra is presented, ranging from the near-ultraviolet (300 nm) to the near-infrared (1.8 mu m). The library spans all the stellar types that are relevant to the integrated light of old and intermediate-age stellar populations in the involved spectral region (spectral types F through M and all luminosity classes). The grid was computed for metallicities ranging from Fe/H = -2.5 to +0.5, including both solar and alpha -enhanced ( alpha /Fe = 0.4) chemical compositions. The synthetic spectra are a good match to observations of stars throughout the stellar parameter space encompassed by the library and over the whole spectral region covered by the computations.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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