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Scaling relations in fossil galaxy groups

✍ Scribed by Habib G. Khosroshahi; Trevor J. Ponman; Laurence R. Jones


Book ID
110841772
Publisher
John Wiley and Sons
Year
2007
Tongue
English
Weight
296 KB
Volume
377
Category
Article
ISSN
0035-8711

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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