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A SAURON view of double-barred galaxies

Published online by Cambridge University Press:  13 April 2010

Adriana de Lorenzo-Cáceres ,
Alexandre Vazdekis ,
Jesús Falcón-Barroso  and
Inma Martínez-Valpuesta
Adriana de Lorenzo-Cáceres
Affiliation:
Instituto de Astrofísica de Canarias, C/ Vía Láctea, S/N, E-38205, La Laguna, Tenerife, Spain email: [email protected]
Alexandre Vazdekis
Affiliation:
Instituto de Astrofísica de Canarias, C/ Vía Láctea, S/N, E-38205, La Laguna, Tenerife, Spain email: [email protected]
Jesús Falcón-Barroso
Affiliation:
Instituto de Astrofísica de Canarias, C/ Vía Láctea, S/N, E-38205, La Laguna, Tenerife, Spain email: [email protected]
Inma Martínez-Valpuesta
Affiliation:
Instituto de Astrofísica de Canarias, C/ Vía Láctea, S/N, E-38205, La Laguna, Tenerife, Spain email: [email protected]
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Double bars might be the key mechanisms to transport gas to the very central regions of galaxies, so double-barred galaxies are key objects to better understand the galaxy formation and evolution scenarios. In order to disentangle the role of double bars in the galaxy build up, we are performing a whole kinematical and stellar population analysis of these objects from high S/N spectroscopic data.

Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 323 - 324
Copyright
Copyright © International Astronomical Union 2010

References

Cervantes, J. L. & Vazdekis, A. 2009, MNRAS, 392, 691CrossRefGoogle Scholar
de Lorenzo-Cáceres, A., Falcón-Barroso, J., Vazdekis, A., & Martínez-Valpuesta, I. 2008, ApJ (Letters), 684, L86CrossRefGoogle Scholar
Vazdekis, A., et al. 2010, MNRAS, in pressGoogle Scholar