Type Center: Sbc
Right: S | Constellation Virgo | |
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Right ascension Center: 14 35 08.763
Left: 14 35 11.0
Right: 14 35 06.354 Declination Center: +05° 21′ 32.41″
Left: +05° 21′ 16″
Right: +05° 21′ 24.41″ Redshift Center: 0.028900
Right: 0.02487 Helio radial velocity Center: 8654
Left: 7483
Right: 7618 Apparent magnitude (B) Center: 14.5
Left: 16
Right: 14.5 Similar Arp 271, Arp 272, UGC 6945, Tadpole Galaxy, NGC 5614 | ||
The NGC 5679 group, also known as Arp 274, is a triplet of galaxies, MCG+1-37-36, MCG+1-37-35 and MCG+1-37-34, spanning about 7005200000000000000♠200000 light-years and at some 400 million light-years from Earth in the constellation Virgo. Arp 247 refers to the Atlas of Peculiar Galaxies, compiled by Halton Arp in 1966. Galaxies 269 through 274 in his catalogue are galaxies that appear to have connected arms.
NGC 6579 was imaged by Hubble in 2009, in a combination of blue, visible, infrared and Hα filters. The photograph shows that all three galaxies, especially the galaxies on the left and right, are starburst galaxies, meaning that there is currently a large amount of star formation in the galaxies. Interstellar dust can be seen between the areas of star formation. Two bright stars can be seen just above the galaxy on the right side; these are foreground stars that are actually part of our own galaxy.
Redshift measurements of the three galaxies give these radial velocity values, from left to right: 7483, 8654, and 7618 km/s. The relatively high redshift for the center galaxy means that it is much farther away - about 65 million light years (20 megaparsecs) behind the other two galaxies. Thus, the center galaxy is likely a background object. The NGC 6579 group was previously thought to be interacting gravitationally, however the newer Hubble image seems to confirm suspicions that the center galaxy is not interacting, as the galaxy arms are not distorted like typical interacting galaxies.