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A&A 402, 865-877 (2003)
DOI: 10.1051/0004-6361:20030034
Gas kinematics of a sample of five Hickson Compact Groups
The data
P. Amram1, H. Plana2, C. Mendes de Oliveira3, C. Balkowski4 and J. Boulesteix11 Observatoire Astronomique Marseille-Provence & Laboratoire d'Astrophysique de Marseille, 2 place Le Verrier, 13248 Marseille Cedex 04, France
2 Observatorio Nacional MCT, Rua General Jose Cristino 77, São Cristóvão, 20921-400 Rio de Janeiro, RJ, Brazil
3 Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, Rua do Matão 1226, Cidade Universitária, 05508-900, São Paulo, SP, Brazil
4 Observatoire de Paris, GEPI, CNRS and Université Paris 7, 5 place Jules Janssen, 92195 Meudon Cedex, France
(Received 9 October 2002 / Accepted 19 December 2002)
Abstract
We present Fabry Perot observations of galaxies in five Hickson
Compact Groups: HCG 10, HCG 19, HCG 87, HCG 91 and HCG 96. We
observed a total of 15 galaxies and we have detected ionized gas
for 13 of them. We were able to derive 2D velocity, monochromatic,
continuum maps and rotation curves for the 13 objects. Almost all
galaxies in this study are late-type systems; only HCG 19a is an
elliptical galaxy. We can see a trend of kinematic evolution
within a group and among different groups - from strongly
interacting systems to galaxies with no signs of interaction -
HCG 10 exhibits at least one galaxy strongly disturbed; HCG 19
seems to be quite evolved; HCG 87 does not show any sign of
merging but a possible gas exchange between two galaxies; HCG 91
could be accreting a new intruder; HCG 96 exhibits past and
present interactions.
Key words: galaxies: kinematics and dynamics -- galaxies: evolution -- galaxies: interactions -- galaxies: ISM -- galaxies: formation -- galaxies: intergalactic medium
Offprint request: P. Amram, Philippe.Amram@oamp.fr
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© ESO 2003
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