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Stellar populations in bulges and disks and the secular evolution connection

Published online by Cambridge University Press:  05 March 2015

Reynier Peletier
Reynier Peletier*
Affiliation:
Kapteyn Institute, GroningenNetherlands, email: [email protected]
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Abstract

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In recent years a considerable amount of new data has become available about stellar populations in the central regions of galaxies. I will discuss what stellar populations can tell us about the formation origin of bulges, and how this relates to the formation of the central regions in giant and dwarf ellipticals. In particular I will concentrate on results from integral field spectroscopy and Spitzer imaging at 3.6, 4.5 and 8 microns.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 336
Copyright
Copyright © International Astronomical Union 2015