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Galaxies and Photometric Signature of Starburst

Published online by Cambridge University Press:  25 May 2016

K.D. Rakos ,
T.I. Maindl  and
J.M. Schombert
K.D. Rakos
Affiliation:
Institut für Astronomie der Universität Wien, Austria
T.I. Maindl
Affiliation:
Institut für Astronomie der Universität Wien, Austria
J.M. Schombert
Affiliation:
NASA HQ, Washington B.C., USA

Extract

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In a series of papers (see Rakos & Schombert 1995, ApJ 439, 47), we have carried out CCD photometry of galaxies in rich clusters at various redshifts. We use a modified Strömgren system, modified in the sense that the filter set is “redshifted” to the cluster of galaxies in consideration (i.e., λobs = λ(1 + z), therefore no k-correction). We call it uz, vz, bz, yz to distinguish it from the original zero redshift system.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 436
Copyright
Copyright © Kluwer 1996