Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S284(7), p. 32-34, 2011
DOI: 10.1017/s1743921312008666
Full text: Unavailable
AbstractThe 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.