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Galaxy in the constellation Camelopardalis

NGC 2146

NGC 2146
All data from the card 15
Constellation
Camelopardalis
Right ascension
06h 18m 37.710s
Declination
+78° 21′ 25.27″
Redshift
0.002999±0.000003
Heliocentric radial velocity
899±1 km/s
Galactocentric velocity
1,043±6 km/s
Distance
63.76 ± 26.62 Mly (19.550 ± 8.161 Mpc)
Apparent magnitude (V)
11.38±0.13
Apparent magnitude (B)
10.59±0.13
Magnitude (J)
8.228±0.020
Magnitude (H)
7.416±0.021
Magnitude (K)
7.063±0.023
Type
SB(s)ab pec; HII;LIRG
Size
119,760 ly(36.72 kpc)(diameter; 25.0 B-mag arcsec−2)124,750 ly × 58,643 ly(38.25 kpc × 17.98 kpc)(diameter; "total" magnitude)
Apparent size (V)
7.97142′ × 3.49228135′

NGC 2146 (also known as the Dusty Hand Galaxy) is a barred spiral galaxy type SB(s)ab pec in the constellation Camelopardalis. The galaxy was discovered in 1876 by Friedrich August Theodor Winnecke.

NGC 2146 has an isophotal diameter of 38.3 kiloparsecs (125,000 light-years), slightly larger than the Milky Way. The galaxy's most conspicuous feature is the dusty lanes of a spiral arm lying across the core of the galaxy as seen from Earth, the arm having been bent 45 degrees by a close encounter with a smaller galaxy, possibly NGC 2146A, about 0.8 billion years ago. This close encounter is credited with the relatively high rates of star formation that qualify NGC 2146 as a starburst galaxy.

Supernovae

SN 2018zd, imaged at Northolt Branch Observatories on 7 March 2018. At that time, the supernova was visible at magnitude +14.0 and brightening.
SN 2018zd, imaged at Northolt Branch Observatories on 7 March 2018. At that time, the supernova was visible at magnitude +14.0 and brightening.

NGC 2146 has been host to three known supernova events:

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Text from Wikipedia, CC BY-SA 4.0 · Source article