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Stellar archeology of the nearby LINER galaxies NGC 4579 and NGC 4736

Published online by Cambridge University Press:  13 April 2010

J. E. Steiner ,
R. B. Menezes ,
T. V. Ricci  and
A. S. de Oliveira
J. E. Steiner*
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, São Paulo - SP, Brasil
R. B. Menezes
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, São Paulo - SP, Brasil
T. V. Ricci
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, São Paulo - SP, Brasil
A. S. de Oliveira
Affiliation:
IPD/Univap
*
†steiner@astro.iag.usp.br
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Abstract

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Stellar archeology of nearby LINER galaxies may reveal if there is a stellar young population that may be responsible for the LINER phenomenon. We show results for the classical LINER galaxies NGC 4579 and NGC 4736 and find no evidence of such populations.

Keywords

Active galactic nucleiLINERSpopulation synthesisspectroscopy
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 430 - 431
Copyright
Copyright © International Astronomical Union 2010

References

Allington-Smith, J. et al. 2002, PASP, 114, 892CrossRefGoogle Scholar
Cid Fernandes, R., Mateus, A., Sodré, L., Stasińska, G., & Gomes, J. M. 2005, MNRAS, 358, 363CrossRefGoogle Scholar
Steiner, J. E., Menezes, R. B., Ricci, T. V., & Oliveira, A. S. 2009, MNRAS, 395, 64CrossRefGoogle Scholar