NGC 459

Spiral galaxy in the constellation Pisces From Wikipedia, the free encyclopedia

NGC 459 is a spiral galaxy in the constellation Pisces.[5] Its velocity with respect to the cosmic microwave background is 12,394±22 km/s, which corresponds to a Hubble distance of 596.2 ± 41.7 Mly (182.80 ± 12.80 Mpc).[1] It was discovered by German-British astronomer William Herschel on 15 October 1784.[4] It was described as being extremely faint by John Dreyer in the New General Catalogue.[5]

Right ascension01h 18m 08.1837s[1]
Declination+17° 33 44.400[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 459
NGC 459 imaged by SDSS
Observation data (J2000 epoch)
ConstellationPisces
Right ascension01h 18m 08.1837s[1]
Declination+17° 33 44.400[1]
Redshift0.0424[2]
Heliocentric radial velocity12705 +/- 5 km/s[1]
Galactocentric velocity12818 +/- 7 km/s[1]
Distance596.2 ± 41.7 Mly (182.80 ± 12.80 Mpc)[1]
Apparent magnitude (V)14.7[3]
Apparent magnitude (B)15.5[3]
Absolute magnitude (V)-21.28[1]
Characteristics
TypeSBc[4]
Apparent size (V)1.0′ × 0.9′[1]
Other designations
2MASX J01180818+1733448, UGC 832, MCG +03-04-017, PGC 4665, CGCG 459-024[3][1]
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Supernova

One supernova has been observed in NGC 459: SN 2011fv (Type II, mag. 18.2) was discovered by F. Ciabattari and E. Mazzoni, as part of the Italian Supernovae Search Project (ISSP), on 26 August 2011.[6][7]

References

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