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). However, four non-redshift measurements give a closer distance of 105.5 Mpc (~344 million light-years). The galaxy was discovered by German-British astronomer William Herschel on 11 April 1785. 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.
Supernovae Two supernovae have been observed in NGC 4375:
SN 1960J (type unknown, mag. 18.5) was discovered by Milton Humason on 18 June 1960. SN 2023vsr (Type II, mag. 17.6478) was discovered by the Zwicky Transient Facility on 24 October 2023.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4375 at Wikimedia Commons NGC 4375 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


