From Wikipedia, the free encyclopedia
NGC 4731
NGC 4731 with legacy surveys
Observation data (J2000 epoch)
Constellation Virgo
Right ascension12h 51m 01.095s [1]
Declination−06° 23′ 34.98″ [1]
Heliocentric radial velocity1488.6 km/s [1]
Distance65 M ly
Apparent magnitude (B)12 [1]
Characteristics
TypeSBc
Other designations
UGCA 302, MCG -01-33-026, PGC 43507 [1]

NGC 4731 is a barred spiral galaxy located near the Virgo supercluster. To its celestial south lies NGC 4731A, a small irregular galaxy. [2] Both galaxies feature high concentrations of neutral HI gas. [3] It is theorized that its elongated arm structure could be related to gravitational interactions with a nearby galaxy, NGC 4967. It is a member of the NGC 4697 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. [4]

See also

New General Catalogue

References

  1. ^ a b c d e "NGC 4731". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ Nemiroff, R.; Bonnell, J., eds. (2010-04-29). "Virgo Cluster Galaxy NGC 4731". Astronomy Picture of the Day. NASA. Retrieved 2022-11-06.
  3. ^ Gottesman, S. T.; Ball, R.; Hunter, J. H.; Huntley, J. M. (1984). "High-resolution observations of the HI content of the barred spiral galaxies NGC 3992 and NGC 4731". The Astrophysical Journal. 286: 471. Bibcode: 1984ApJ...286..471G. doi: 10.1086/162622.
  4. ^ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
From Wikipedia, the free encyclopedia
NGC 4731
NGC 4731 with legacy surveys
Observation data (J2000 epoch)
Constellation Virgo
Right ascension12h 51m 01.095s [1]
Declination−06° 23′ 34.98″ [1]
Heliocentric radial velocity1488.6 km/s [1]
Distance65 M ly
Apparent magnitude (B)12 [1]
Characteristics
TypeSBc
Other designations
UGCA 302, MCG -01-33-026, PGC 43507 [1]

NGC 4731 is a barred spiral galaxy located near the Virgo supercluster. To its celestial south lies NGC 4731A, a small irregular galaxy. [2] Both galaxies feature high concentrations of neutral HI gas. [3] It is theorized that its elongated arm structure could be related to gravitational interactions with a nearby galaxy, NGC 4967. It is a member of the NGC 4697 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. [4]

See also

New General Catalogue

References

  1. ^ a b c d e "NGC 4731". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ Nemiroff, R.; Bonnell, J., eds. (2010-04-29). "Virgo Cluster Galaxy NGC 4731". Astronomy Picture of the Day. NASA. Retrieved 2022-11-06.
  3. ^ Gottesman, S. T.; Ball, R.; Hunter, J. H.; Huntley, J. M. (1984). "High-resolution observations of the HI content of the barred spiral galaxies NGC 3992 and NGC 4731". The Astrophysical Journal. 286: 471. Bibcode: 1984ApJ...286..471G. doi: 10.1086/162622.
  4. ^ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.

Videos

Youtube | Vimeo | Bing

Websites

Google | Yahoo | Bing

Encyclopedia

Google | Yahoo | Bing

Facebook