Constraining stellar populations with high resolution spectra

Details Constraining stellar populations with high resolution spectra Constraining stellar populations with high resolution spectra

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..551o&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

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Scientific paper

We propose a method for recovering the star formation history of a
population from its observed high or medium resolution spectrum. We then
discuss the data quality needed for such a reconstruction to be reliable
in a general, method independent context and finally show some
applications.

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