NGC 4615

Galaxy in the constellation Coma Berenices From Wikipedia, the free encyclopedia

NGC 4615 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 5,022±20 km/s, which corresponds to a Hubble distance of 241.6 ± 16.9 Mly (74.07 ± 5.19 Mpc).[1] However, one non-redshift measurement gives a much closer distance of 213 Mly (65.4 Mpc).[2] It was discovered by German astronomer Heinrich d'Arrest on 9 May 1864.[3]

NGC 4615 and NGC 4614 imaged by SDSS
Right ascension12h 41m 37.3313s[1]
Declination+26° 04 21.871[1]
Redshift0.015797±0.0000112[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 4615
NGC 4615 imaged by SDSS
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 41m 37.3313s[1]
Declination+26° 04 21.871[1]
Redshift0.015797±0.0000112[1]
Heliocentric radial velocity4,736±3 km/s[1]
Distance213 Mly (65.4 Mpc)[1]
Group or clusterHolm 439
Apparent magnitude (V)13.84[1]
Characteristics
TypeScd[1]
Size~160,400 ly (49.17 kpc) (estimated)[1]
Apparent size (V)1.6′ × 0.7′[1]
Other designations
HOLM 439A, IRAS 12391+2620, 2MASX J12413730+2604223, Arp 34, UGC 7852, MCG +04-30-013, PGC 42584, CGCG 129-018[1]
Close

NGC 4615 is listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 34, as an example of a galaxy that looks like a stretched-out S shape.[4]

NGC 4615 and NGC 4614 are listed together as Holm 439 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[5] This grouping was also listed by A. P. Mahtessian in a paper published in 1998.[6]

Supernovae

Two supernovae have been observed in NGC 4615:

  • SN 1987F (Type II-P, mag. 15.8) was discovered independently by Natalya Metlova on 22 April 1987, and by Thomas Schildknecht [de] on 23 April 1987.[7][8][9]
  • SN 2025nzi (Type Ib, mag. 19.016) was discovered by ATLAS on 18 June 2025.[10]

See also

References

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