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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*
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
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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.

Type
Poster Papers
Copyright
Copyright © International Astronomical Union 2010

References

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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