Studying Stellar Populations at High Spectral Resolution

Details Studying Stellar Populations at High Spectral Resolution Studying Stellar Populations at High Spectral Resolution

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26..109b&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Galaxies: Evolution, Galaxies: Stellar Content

Scientific paper

I describe very briefly the new libraries of empirical spectra of stars covering wide ranges of values of the atmospheric parameters T_{eff}, log g, [Fe/H], as well as spectral type, that have become available in the recent past, among them the HNGSL, MILES, UVES-POP, ELODIE, and the IndoUS libraries. These libraries are complementary in spectral resolution and wavelength coverage, and will prove extremely useful to describe spectral features expected in galaxy spectra from the NUV to the NIR. The fits to observed galaxy spectra using stellar population models are discussed.

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