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Photometry of Hickson Compact Group N.90

Published online by Cambridge University Press:  26 July 2016

G. Longo ,
H. Lorenz ,
G. Richter  and
G. Busarello
G. Longo
Affiliation:
Osservatorio Astronomico di Capodimonte, via Moiariello 16, I-80131 Napoli, Italy
H. Lorenz
Affiliation:
Astrophysicalisches Institut Potsdam, An der Sternwarte 16, D-14482, Potsdam-Babelsberg, Germany
G. Richter
Affiliation:
Astrophysicalisches Institut Potsdam, An der Sternwarte 16, D-14482, Potsdam-Babelsberg, Germany
G. Busarello
Affiliation:
Osservatorio Astronomico di Capodimonte, via Moiariello 16, I-80131 Napoli, Italy

Abstract

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Deep CCD photometry and kinematical observations can be used to constrain the dynamical status of compact groups of galaxies. In the case of Hickson 90 the main interaction is taking place between NGC 7174 and NGC 7173 while NGC 7176 appears to be virtually undisturbed.

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 619 - 622
Copyright
Copyright © Kluwer 1994 

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