# Shakhbazian compact galaxy groups - II. Photometric and spectroscopic study of ShCG 376

@article{Tovmassian2003ShakhbazianCG,
title={Shakhbazian compact galaxy groups - II. Photometric and spectroscopic study of ShCG 376},
author={Hrant M. Tovmassian and Heinz Tiersch and Vahram Chavushyan and Gaghik H. Tovmassian},
journal={Astronomy and Astrophysics},
year={2003},
volume={401},
pages={463-470}
}
The results of the redshift measurements and of the detailed surface photometry in BVR of the compact group ShCG 376 are presented. The radial velocity dispersion, the virial mass, the total luminosity, the ${\cal M}/L$ ratio, and the crossing time of the group are estimated. The group consists of eight accordant redshift spiral galaxies. Four (or possibly five) of the group members have emission-line spectra. Such morphological content and the number of emission-line galaxies are very atypical…
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## References

SHOWING 1-10 OF 34 REFERENCES
Shakhbazian compact galaxy groups - I. Photometric, spectroscopic and X-ray study of ShCG 154, ShCG 166, ShCG 328, ShCG 360
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 dierent
Shakhbazian compact groups: Poor clusters of galaxies
• Physics
• 2001
The environment of 105 elongated ($b/a< 0.5$) ShCGs is investigated for galaxies probably associated with them. Counts of galaxies are made in two reciprocally orthogonal stripes of $5\arcmin$ width
Far-infrared emission from Shakhbazian Compact Galaxy Groups
• Physics
• 1998
Using the IRAS archives, we searched for far-infrared (FIR) counterparts of Shakh bazian Compact Groups of Galaxies (SCGGs). Reliable IRAS detections are identified at the positions of 24 out of 367
Systematic properties of compact groups of galaxies.
One hundred compact groups of galaxies have been identified by a systematic search of the Palomar Observatory Sky Survey red prints. Each group contains four or more galaxies within a 3 mag range,
Radio Emission of Shakhbazian Compact Galaxy Groups
We detect 353 radio sources from the NRAO VLA Sky Survey (NVSS) and the FIRST Survey within the areas of 179 Shakhbazian compact groups (ShCGs) of galaxies. Ninety-three of them are identi—ed with
The remarkable cluster Shakhbazian I.
• Physics
• 1973
A plate of the compact cluster of galaxies Shakhbazian I is shown and described. Various possible models for the cluster are analyzed. We conclude, as did Robinson and Wampler (1973), that it is most
Properties of dense galaxy groups and the implications of their existence
Galaxy counts are reported within 1 deg of the 100 dense groups cataloged by Hickson (1982). The results suggest that a much smaller fraction of the groups can be explained as chance alignments than
The Dynamical Status of Stephan's Quintet
• Physics
• 1997
Multiwavelength data for Stephan's Quintet (SQ) are consistent with the following model for this compact galaxy group. (1) Discordant-redshift NGC 7320 is an unrelated foreground galaxy. (2) In the