Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-07T23:18:50.950Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar population history of Seyfert 2 nuclei

Published online by Cambridge University Press:  24 November 2004

R. Rodrigues Lacerda ,
R. Cid Fernades ,
Q. Gu ,
J. Melnick ,
E. Terlevich ,
R. Terlevich  and
D. Kunth
R. Rodrigues Lacerda
Affiliation:
Universidade Federal de Santa Catarina, Florianópolis-SC, Brazil
R. Cid Fernades
Affiliation:
Universidade Federal de Santa Catarina, Florianópolis-SC, Brazil
Q. Gu
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, P. R. China
J. Melnick
Affiliation:
European Southern Observatory, Alonso de Codorva 3107, Santiago, Chile
E. Terlevich
Affiliation:
INAOE, Tonantzintla, Puebla, Mexico
R. Terlevich
Affiliation:
INAOE, Tonantzintla, Puebla, Mexico Institute of Astronomy, Madingley Road, CB3 OHA Cambridge, UK
D. Kunth
Affiliation:
Institut d'Astrophysique de Paris, 98bis Bouleward Arago, 75014 Paris, France
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the results of a new stellar population synthesis code which mixes both evolutionary and empirical population synthesis techniques. The code decomposes a given galaxy spectrum into a base of high resolution spectra from the recent evolutionary synthesis models of Bruzual & Charlot (2003). The main novelty is that now we synthesize the whole Fλ spectrum, rather than a handful of absorption lines and colors.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. 187 - 188
Copyright
© 2004 International Astronomical Union