NGC 2655

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NGC 2655
250px
Observation data (J2000 epoch)
Constellation Camelopardalis
Right ascension 08h 55m 37.7s[1]
Declination +78° 13′ 03″[1]
Redshift 1400 ± 1 km/s[1]
Distance 63 Mly (19.5 Mpc)[1]
Type SAB(s)0/a [1]
Apparent dimensions (V) 4′.9 × 4′.1[1]
Apparent magnitude (V) 10.1
Other designations
Arp 225, UGC 4637, PGC 25069[1]
See also: Galaxy, List of galaxies

NGC 2655 is a lenticular galaxy in the constellation Camelopardalis. It is at a distance of 60 million light years from Earth. NGC 2655 is a Seyfert galaxy. The galaxy has asymmetric dust lanes in the centre of the galaxy, tidal arms and extended neutral hydrogen gas and may have experienced recently a merger. The complex dynamics of the HI and optical tails suggest the galaxy may have undergonen more mergers in the past. a weak bar has been detected in infrared H band. The diametre of the disk of the galaxy is estimated to be 60 Kpc (195,000 ly).[2]

William Herschel discovered NGC 2655 in September 26, 1802 and descripted it as very bright and considerably large. The galaxy can be glimsed with a 4 inches telescope under dark skies nearly 10° from the north celestial pole.[3] One supernova has been observed in NGC 2655, SN 2011B,[4] a type Ia with peak magnitude 12.8.[5]

NGC 2655 is the brightest member of NGC 2655 group, which also contains the Sc galaxy NGC 2715, NGC 2591, and NGC 2748.[6][7] One of the gas structures of NGC 2655 is traling off toward the small galaxy UGC 4714.[2]

References

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  4. List of Supernovae IAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
  5. List of supernovae sorted by Magnitude for 2011
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External links