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The shapes of Shakhbazian compact groups of galaxies

✍ Scribed by H. Oleak; D. Stoll; H. Tiersch; H. T. Macgillivray

Publisher: John Wiley and Sons
Year: 1998
Tongue: English
Weight: 337 KB
Volume: 319
Category: Article
ISSN: 0004-6337
DOI: 10.1002/asna.2123190404

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## Abstract Numerical simulations as well as optical and X‐ray observations over the last few years have shown that poor groups of galaxies can evolve to what is called a fossil group. Dynamical friction as the driving process leads to the coalescence of individual galaxies in ordinary poor groups