NGC 7124 explained

NGC 7124
Constellation Name:Indus
Epoch:J2000
Type:SB(rs)bc[1]
Dist Ly:NaNMpc
Z:0.017251
H Radial V:5172 ± 8 km/s
Appmag V:12.3
Size V:2.8' x 1.1'
Size:~63.21kpc (estimated)
Names:, ESO 237- G 002

NGC 7124 is a large spiral galaxy in the constellation of Indus. Its velocity with respect to the cosmic microwave background is 4988 ± 15 km/s, which corresponds to a Hubble distance of 73.57 ± 5.16 Mpc (∼240 million light-years). It was discovered by British astronomer John Herschel on 8 July 1834.[2]

NGC 7124 is classified as a LINER galaxy, i.e. it has a type of nucleus that is defined by its spectral line emission which has weakly ionized or neutral atoms, while the spectral line emission from strongly ionized atoms is relatively weak..

One supernova has been observed in NGC 7124: SN 2023pwl (type Ia, mag 16.7).[3]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 7124 . 6 August 2024.
  2. https://cseligman.com/text/atlas/ngc71.htm#7124 Celestial Atlas entry for NGC 7124.
  3. https://www.wis-tns.org/object/2023pwl Transient Name Server entry for SN 2023pwl.