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S0 Galaxy Line Strengths and Gradients

Published online by Cambridge University Press:  25 May 2016

David Fisher ,
Marijn Franx  and
Garth Illingworth
David Fisher
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Marijn Franx
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Garth Illingworth
Affiliation:
UCO/Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz

Extract

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Line strengths and their gradients in Mg, Fe, and Hβ have been determined for a sample of 20 S0 galaxies in order to study the stellar populations of their bulges and disks and to investigate their relationship to elliptical galaxies. The data were obtained with the Lick Observatory 3m telescope in the long-slit mode over the region 4215–5615 Å with resolution 3.1 Å.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 374
Copyright
Copyright © Kluwer 1996