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Stellar population synthesis in AGNs
Published online by Cambridge University Press: 24 November 2004
Abstract
We present a numerical code to synthesize the stellar population of galaxies, using the observed flux as observable, for the visible and IR range This code is an evolution of a previous one, which used the equivalent widths.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
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- Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 169 - 170
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- © 2004 International Astronomical Union