Group of Galaxies Hickson 40 (Arp 321)

Hickson 40
Hickson 40: Image taken with the Hubble Space Telescope. © 2022 NASA, ESA and STScI [565]


In 1959 the Russian astronomer Boris Vorontsov-Velyaminov published his «Atlas and Catalogue of Interacting Galaxies». This group of galaxies is referred as VV 116. [432]

Few years later in 1966 the American astronomer Halton Christian Arp published his «Atlas of Peculiar Galaxies», which was the result of more than four years of direct photography with the 200-inch Hale telescope of Mount Wilson and Palomar Observatories. He collected 338 unusual looking galaxies or group of galaxies. He ordered them empirically according to their form and visual appearance. Part of his discoveries was based on the Vorontsov-Velyaminov catalogue. This group of galaxies with the number 321 was arranged in group #311-321 as groups of galaxies. He noted: «VV position. Sharp absorption lane in connection to southern galaxy.» [199]

The British-Canadian astronomer Paul Hickson presented in 1982 his systematic search for groups of galaxies on the photo plates of the Palomar Observatory Sky Survey (POSS) to the public. In order to be classified by him as a galaxy group, at least four members should be identifiable, which had to be reasonably compact and isolated from the rest. The catalog contains 100 groups of galaxies. [140] The group originally had 6 members (A through F) but F was a misidentified foreground star. In the 1993 special issue of his «Atlas of Compact Groups of Galaxies» it was dropped. There he wrote «This famous and beautifoul group is also known as Arp 321 and VV 116. It is a very compact quintet of overlapping galaxies. Three galaxies are radio sources; the faintest galaxy has infrared emission.» [166]

Physical Properties

This quintet includes three spiral-shaped galaxies, an elliptical galaxy and a lenticular (lens-like) galaxy in a moment as they fall together before they merge in about one billion (109) years. The galaxies are so crowded, that they occupy a space less than twice the diameter of our Milky Way’s stellar disc. Almost every one of the galaxies has a compact radio source at its core, which could be evidence for the presence of a supermassive black hole. X-ray observations show that the galaxies have been gravitationally interacting as witnessed by the presence of a lot of hot gas amongst them. Infrared observations reveal clues to the rate of formation of new stars. [565]

«Catalogue of Principal Galaxies» Paturel et al., 1989 [144]
PGC RA Dec Type Dim Btot HRV PA Names
PGC 27508 09 38 53.2 -04 51 34 SB M 1.1 x .3 15.9 6853 61 MCG 1-25-8, (VV 116), (ARP 321), IRAS 9364-437, ANON 936-4C, HICK 40C
PGC 27509 09 38 53.5 -04 50 56 E M 1.3 x 1.0 13.7 6622 175 MCG 1-25-9, (VV 116), (ARP 321), ANON 936-4A, HICK 40A
PGC 27513 09 38 55.0 -04 51 58 L M 1.1 x .7 14.9 6821 125 MCG 1-25-10, (VV 116), (ARP 321), ANON 936-4B, HICK 40B
PGC 27515 09 38 55.5 -04 51 28 S M .7 x .3 17.3 6625 125 MCG 1-25-11, (VV 116), (ARP 321), ANON 936-4E, HICK 40E
PGC 27516 09 38 55.8 -04 50 14 SB M .9 x .4 15.1 6466 80 MCG 1-25-12, (VV 116), (ARP 321), ANON 936-4D, HICK 40D
PGC 27517 09 38 56.5 -04 50 23 E M  x  HICK 40F

Finder Chart

The Hickson 40 compact group of galaxies can be found in the long constellation Hydra near the constellation Sextans, between the stars ι Hydrae (3.91 mag) and α Hydrae (Alphard, 1.98 mag). The best time for observation is in the months from December to May.

Finder Chart Group of Galaxies Hickson 40 (Arp 321)
Group of Galaxies Hickson 40 (Arp 321) in constellation Hydra. Charts created using SkySafari 6 Pro and STScI Digitized Sky Survey. Limiting magnitudes: Constellation chart ~6.5 mag, DSS2 close-ups ~20 mag. [149, 160]

More Objects Nearby (±15°)