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A&A 392, 33-52 (2002)
DOI: 10.1051/0004-6361:20020877
Shakhbazian compact galaxy groups
I. Photometric, spectroscopic and X-ray study of ShCG 154, ShCG 166, ShCG 328, ShCG 360
H. Tiersch1, H. M. Tovmassian2, D. Stoll1, A. S. Amirkhanian3, S. Neizvestny4, H. Böhringer5 and H. T. MacGillivray61 Sternwarte Königsleiten, 81477 München, Leimbachstr. 1a, Germany
2 Instituto Nacional de Astrofísica Optica y Electrónica, Apartado Postal 51 y 216, CP 72000, Puebla, Pue., México
e-mail: hrant@inaoep.mx
3 Byurakan Astrophysical Observatory, NAS, Armenia
e-mail: vachik@nssp-gov.am
4 Special Astrophysical Observatory, RAS, Nizhny Arkhyz, Russia
e-mail: neiz@sao.ru
5 MPI Extraterrestrische Physik, Garching, Germany
e-mail: hxb@mpe.mpg.de
6 Royal Observatory, Edinburg, UK
e-mail: hmg@roe.ac.uk
(Received 3 September 2001 / Accepted 18 April (2002) )
Abstract
Shakhbazian compact galaxy groups belong to the interesting class of
compact groups. Because of their large number (the catalogue contains 377
entries) we are able to study the groups in different stages of evolution. Here
we give the results of detailed study of four groups, ShCG 154, ShCG 166, ShCG
328 and ShCG 360. We present the redshifts of individual galaxies in groups,
the results of the surface photometry in
BVR, the contourplots of the surface
brightness versus effective radius of galaxies, the twisting postion angle versus effective radius of galaxies, the radial
velocity
dispersions, the crossing times, the mass-to-luminosity ratios of groups and the
results of the X-ray study. The dynamical state of groups, interactions between
member galaxies, and the physical parameters of groups are discussed.
Key words: galaxies: clusters: general -- galaxies: interactions -- galaxies: kinematics and dynamics -- galaxies: photometry -- X-rays: galaxies
Offprint request: H. Tiersch, htiersch@uni.de
SIMBAD Objects
© ESO 2002
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