Quote from Paul Hickson's Atlas
of Compact Groups of Galaxies:
"Group 56 consists of five galaxies, three of which appear to be in contract and interacting. Two of these three galaxies (B and D) are radio sources. Infrared emission is also detected from this interacting system."
This interesting group, found in the Constellation of Ursa Major, belongs both to the list of Vorontsov-Vel'yaminov (1959; number 150) and to that of Arp (1966; number 322). It is characterized by the spectacular stream of matter linking galaxies B and C. Galaxy C shows a conspicuous asymmetric halo but galaxy D has a simple outer luminosity profile. Finally, we note that galaxy A and galaxy D are Seyfert galaxies.
Based on their red shift, a rough distance estimate for the Hickson 56 galaxies is 425 million light years.
Classification: Sbc, Edge-on
Spiral |
Classification: SB0, Barred Lenticular
|
Classification: (R')S0/a pec:, pseudo outer ring, Lenticular, peculiar (uncertain) |
Classification: SA(s)0/a pec: Sy2, Spiral, S-shaped, peculiar (uncertain), Seyfert Type II |
Classification: SB0 pec:, Barred Lenticular, peculiar (uncertain) |
Hickson 56 is also listed
as:
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George Normandin, KAS
May 15th, 2002