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Stellar Populations in Barred Galaxies

Published online by Cambridge University Press:  13 April 2010

C. Robert ,
S. Cantin ,
M. Mollá ,
A. Pellerin  and
É. Brière
C. Robert
Affiliation:
Université Laval & CRAQ, Québec, QC G1V 0A6, Canada, carobert@phy.ulaval.ca
S. Cantin
Affiliation:
Université Laval & CRAQ, Québec, QC G1V 0A6, Canada, carobert@phy.ulaval.ca
M. Mollá
Affiliation:
Departamento de Investigación Básica, CIEMAT Avda. Complutense 22, 28040 Madrid, Spain
A. Pellerin
Affiliation:
Texas A&M University, Dept of Physics & Astronomy, College Station, TX 77843, USA
É. Brière
Affiliation:
Université Laval & CRAQ, Québec, QC G1V 0A6, Canada, carobert@phy.ulaval.ca
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Abstract

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We developed an iterative technique to better characterize stellar populations and the central activity of barred galaxies using evolutionary synthesis codes and OASIS data. The case of NGC 5430 is presented here. Our results are reinforcing the role played by the bar and nuclear structures for the evolution of galaxies.

Keywords

galaxies: spiralgalaxies: stellar contentgalaxies: bulgesgalaxies: evolution
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 418 - 419
Copyright
Copyright © International Astronomical Union 2010

References

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