NGC 1633

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Right ascension04h 40m 09.1088s[1]
Declination+07° 20 58.172[1]
Redshift0.016632±0.00000700[1]
NGC 1633
NGC 1633 and NGC 1634 imaged by Pan-STARRS
Observation data (J2000 epoch)
ConstellationTaurus
Right ascension04h 40m 09.1088s[1]
Declination+07° 20 58.172[1]
Redshift0.016632±0.00000700[1]
Heliocentric radial velocity4,986±2 km/s[1]
Distance187.87 ± 5.23 Mly (57.600 ± 1.604 Mpc)[1]
Group or clusterNGC 1762 Group (LGG 120)
Apparent magnitude (V)14.36[1]
Characteristics
TypeSAB(s)ab[1]
Size~68,900 ly (21.14 kpc) (estimated)[1]
Apparent size (V)1.0′ × 0.9′[1]
Other designations
HOLM 079A, IRAS 04374+0715, 2MASX J04400910+0720577, UGC 3125, MCG +01-12-014, PGC 15774, CGCG 419-023[1]

NGC 1633 is an intermediate spiral galaxy in the constellation of Taurus. Its velocity with respect to the cosmic microwave background is 4,930±4 km/s, which corresponds to a Hubble distance of 237.1 ± 16.6 Mly (72.71 ± 5.09 Mpc).[1] However, three non-redshift measurements give a closer mean distance of 187.87 ± 5.23 Mly (57.600 ± 1.604 Mpc).[2] It was discovered by German-British astronomer William Herschel on 9 December 1798.[3][4]

NGC 1633 is a member of NGC 1762 group (also known as LGG 120). This group contains 27 galaxies, including NGC 1590, NGC 1642, NGC 1691 [fr], NGC 1713 [fr], NGC 1719, NGC 1762, and IC 392 [de].[5][6]

Supernova

One supernova has been observed in NGC 1633:

See also

References

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