Astronomy:NGC 4375

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NGC 4375
File:250px
NGC 4375 imaged by SDSS
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 25m 00.4734s[1]
Declination+28° 33′ 30.952″[1]
Redshift0.030153 [1]
Helio radial velocity9040 ± 3 km/s[1]
Distance448.6 ± 31.4 Mly (137.54 ± 9.63 Mpc)[1]
Apparent magnitude (V)12.6[1]
Characteristics
TypeSB(r)ab pec?[1]
Size~148,000 ly (45.37 kpc) (estimated)[1]
Apparent size (V)1.4′ × 1.2′[1]
Other designations
IRAS 12224+2850, UGC 7496, MCG+05-29-080, PGC 40449[1]

NGC 4375 is a barred spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 9325 ± 20 km/s, which corresponds to a Hubble distance of 137.54 ± 9.63 Mpc (~448 million light-years).[1] However, four non-redshift measurements give a closer distance of 105.5 Mpc (~344 million light-years).[2] The galaxy was discovered by German-British astronomer William Herschel on 11 April 1785.[3]

The SIMBAD database lists NGC 4375 as a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[4]

Supernovae

Two supernovae have been observed in NGC 4375:

See also

References