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NGC 1961

Galaxy in the constellation Camelopardis From Wikipedia, the free encyclopedia

NGC 1961
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NGC 1961 is a spiral galaxy in the constellation Camelopardalis. It was discovered by German-British astronomer William Herschel on 3 December 1788.[2] It was also observed by Guillaume Bigourdan on 22 December 1891, causing it to be listed in the Index Catalogue as IC 2133.[2] Its velocity with respect to the cosmic microwave background for is 3,909±2 km/s, which corresponds to a Hubble distance of 188.0 ± 13.2 Mly (57.65 ± 4.04 Mpc).[1] However, seven non redshift measurements give a much closer distance of 145.42 ± 27.36 Mly (44.586 ± 8.390 Mpc).[3]

Quick facts Observation data (J2000 epoch), Constellation ...

The galaxy has been distorted, however no companion has been detected nor double nuclei that could show a recent merger. Its outer arms are highly irregular. Two long straight arms extend from the north side of the galaxy.[4] A luminous X-ray corona has been detected around the galaxy.[5][6] NGC 1961 is the central member of the small group of nine galaxies, the NGC 1961 group.[4]

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Supernovae

Four supernovae have been observed in NGC 1961:

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References

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