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Stellar population synthesis in AGNs

Published online by Cambridge University Press:  24 November 2004

J. Frémaux ,
C. Boisson ,
M. Joly  and
D. Pelat
J. Frémaux
Affiliation:
LUTH, Observatoire de Paris, F-92195 Meudon, France email: julien.fremaux@obspm.fr
C. Boisson
Affiliation:
LUTH, Observatoire de Paris, F-92195 Meudon, France email: julien.fremaux@obspm.fr
M. Joly
Affiliation:
LUTH, Observatoire de Paris, F-92195 Meudon, France email: julien.fremaux@obspm.fr
D. Pelat
Affiliation:
LUTH, Observatoire de Paris, F-92195 Meudon, France email: julien.fremaux@obspm.fr
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Abstract

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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

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 169 - 170
Copyright
© 2004 International Astronomical Union