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Stellar Populations in the Center of the Barred Galaxy NGC 4900

Published online by Cambridge University Press:  01 December 2006

Simon Cantin ,
Mercedes Mollá ,
Carmelle Robert  and
Anne Pellerin
Simon Cantin
Affiliation:
Université Laval and Observatoire du mont Mégantic, Québec (Canada), G1K 7P4 email: simon.cantin.1@ulaval.ca
Mercedes Mollá
Affiliation:
CIEMAT, Avda. Complutense 22, 28040 Madrid (Spain)
Carmelle Robert
Affiliation:
Université Laval and Observatoire du mont Mégantic, Québec (Canada), G1K 7P4 email: simon.cantin.1@ulaval.ca
Anne Pellerin
Affiliation:
Space Telescope Science Institute, Baltimore (USA)
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Abstract

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We characterize the stellar populations in the nuclear region of the barred spiral galaxy NGC 4900 using the integral field spectrometer OASIS and the synthesis code LavalSB and the code from Mollá & García-Vargas (2000) for the young (<10 Myr) and the old stellar populations, respectively. The high spatial resolution of the instrument allows us to find an old population uniformely distributed and younger regions located at the end of the galaxy bar and on each side of a nuclear bar.

Keywords

Stellar populationsGalaxies: spiralGalaxies: barredGalaxies: Abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 499 - 500
Copyright
Copyright © International Astronomical Union 2007

References

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