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NGC 767

From Wikipedia, the free encyclopedia
Galaxy located in the constellation Cetus
NGC 767
SDSS image of NGC 767
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 01h 58m 50.822s
Declination −09° 35′ 13.61″
Redshift 0.01805[1]
Heliocentric radial velocity 5362 km/s[1]
Distance 246.5 ± 17.3 Mly (75.58 ± 5.3 Mpc)[2]
Apparent magnitude (B)14[1]
Characteristics
Type SBb pec?[2]
Other designations
MCG -02-06-010, PGC 7483[1]

NGC 767 is a barred spiral galaxy located in the constellation Cetus about 241 million light years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.[3] [4] [5]

One supernova has been observed in NGC 767: SN 2019lre (type II, mag. 19.2).[6]

See also

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References

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  1. ^ a b c d "NGC 767". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020年05月24日.
  2. ^ a b "Results for object NGC 0767 (NGC 767)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020年05月24日.
  3. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020年03月30日.
  4. ^ "Revised NGC Data for NGC 767". spider.seds.org. Retrieved 2020年03月30日.
  5. ^ Ford, Dominic. "The galaxy NGC 767 - In-The-Sky.org". in-the-sky.org. Retrieved 2020年03月30日.
  6. ^ "SN 2019lre". Transient Name Server. IAU . Retrieved 6 September 2024.
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  • Media related to NGC 767 at Wikimedia Commons
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