NGC 3557

NGC 3557
Observation data (J2000 epoch)
ConstellationCentaurus
Right ascension11h 09m 57.6396s
Declination−37° 32′ 21.037″
Redshift0.010270
Heliocentric radial velocity3079 ± 6 km/s
Distance163.5 ± 11.5 Mly (50.12 ± 3.53 Mpc)
Apparent magnitude (V)10.4
Characteristics
TypeE3
Size~246,200 ly (75.48 kpc) (estimated)
Apparent size (V)4.0′ × 3.0′
Other designations
ESO 377- G 016, 2MASX J11095583-3732345, MCG -06-25-005, PGC 33871

NGC 3557 is a large elliptical galaxy in the constellation of Centaurus. Its velocity with respect to the cosmic microwave background is 3398 ± 23 km/s, which corresponds to a Hubble distance of 50.12 ± 3.53 Mpc (~163 million light-years). However, 20 non-redshift measurements give a distance of 32.905 ± 2.289 (~107 million light-years). The galaxy was discovered by British astronomer John Herschel on 21 April 1835.

The SIMBAD database lists NGC 3557 as a Seyfert I 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. Additionally, NED lists NGC 3557 as a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.

NGC 3557 Group

NGC 3557 is the largest and brightest galaxy in a group of galaxies that bears its name. The NGC 3557 group (also known as LGG 229) includes at least eleven galaxies, including NGC 3533 [fr], NGC 3557B [d], NGC 3564 [fr], NGC 3568 and NGC 3573 [fr].

Supernova

One supernova has been observed in NGC 3557.

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 "Results for object NGC 3557". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 11 August 2024.
  2. ↑ "Distance Results for NGC 3557". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 11 August 2024.
  3. ↑ Seligman, Courtney. "NGC 3557". Celestial Atlas. Retrieved 11 August 2024.
  4. ↑ "NGC 3557". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 December 2024.
  5. ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
  6. ↑ "SN 2023bpx". Transient Name Server. IAU. Retrieved 11 August 2024.