Physical requirements for modeling stellar atmospheres according to the different spectral features observed

Details Physical requirements for modeling stellar atmospheres according to the different spectral features observed Physical requirements for modeling stellar atmospheres according to the different spectral features observed

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..241...91c&link_type=ejournal

Stellar Populations as Building Blocks of Galaxies, Proceedings of IAU Symposium #241. Edited by A. Vazdekis and R. F. Peletier

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