NGC 2146
NGC 2146 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.[2]
NGC 2146 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Camelopardalis |
Right ascension | 06h 18m 37.7s[1] |
Declination | +78° 21′ 25″[1] |
Redshift | 893 ± 5 km/s[1] |
Distance | 70,000,000 lyr |
Apparent magnitude (V) | 11.38[1] |
Characteristics | |
Type | SB(s)ab pec[1] |
Apparent size (V) | 6′.0 × 3′.4[1] |
Other designations | |
UGC 3429,[1] CGCG 348-017, MCG +13-05-0, 4C +78.06, PGC 18797[1] |
It has a diameter of 80,000 lyr.[2] 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.[2] This close encounter is credited with the relatively high rates of star formation that qualify NGC 2146 as a starburst galaxy.[2]
It has been host to two known supernova events:
Gallery
- SN 2018zd, imaged at Northolt Branch Observatories on 7 March 2018. At that time, the supernova was visible at magnitude +14.0 and brightening.[7]
References
- NED (July 16, 2012), Results for search on NGC 2146
- "Feeling the strain". The Hubble European Space Agency Information Centre. 22 August 2011. Retrieved 6 October 2012.
- Mattlla, S; Greimel, R; Meikle, P (2005). "LIRIS Discovers Supernovae in Starburst Galaxies" (PDF). The Newsletter of the Isaac Newton Group of Telescopes. 9: 16. Bibcode:2005INGN....9...16M. Retrieved 8 July 2015.
- "Image of supernova 2005V". rochesterastronomy.org. 4 February 2005. Retrieved 10 March 2018.
- Zhang, Jujia; Xu, Liang; Wang, Xiaofeng (6 March 2018). "ATEL #11379: Spectroscopic Classification of SN 2018zd as a very young Type IIn Supernova". Retrieved 10 March 2018.
- "SN 2018zd". Transient Name Server. 2 March 2018. Retrieved 10 March 2018.
- "Supernova 2018zd in NGC 2146". rochesterastronomy.org. 2 March 2018. Retrieved 10 March 2018.
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