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A first glance into the Spectral Energy Distributions of Single Stellar Populations in the Infrared range

Published online by Cambridge University Press:  17 August 2012

Sofia Meneses-Goytia  and
Reynier F. Peletier
Sofia Meneses-Goytia
Affiliation:
Kapteyn Instituut, Rijksuniversiteit Groningen, Landleven 12, 9747AD, Groningen, the Netherlands email: s.meneses-goytia@astro.rug.nl
Reynier F. Peletier
Affiliation:
Kapteyn Instituut, Rijksuniversiteit Groningen, Landleven 12, 9747AD, Groningen, the Netherlands email: s.meneses-goytia@astro.rug.nl
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Abstract

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The present work shows the Spectral Energy Distributions (SEDs) in the infrared using the IRTF stellar library, obtained using models based on Single Stellar population Models (SSP). We have focused on the K band in order to compare with observables of elliptical galaxies. We also present the comparisons of our models with velocity dispersions, ages and metallicities obtained with models in the optical range.

Keywords

infrared: starsgalaxiesgalaxies: formationelliptical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 32 - 34
Copyright
Copyright © International Astronomical Union 2012

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