Astronomy:NGC 7321

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NGC 7321
NGC 7321 imaged by SDSS
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension 22h 36m 28.0108s[1]
Declination+21° 37′ 18.648″[1]
Redshift0.023843±0.0000120[1]
Helio radial velocity7,148±4 km/s[1]
Distance297.50 ± 14.14 Mly (91.214 ± 4.334 Mpc)[2]
Apparent magnitude (V)13.71[1]
Characteristics
TypeSB(r)b[1]
Size~147,100 ly (45.11 kpc) (estimated)[1]
Apparent size (V)1.6′ × 1.1′[1]
Other designations
HOLM 793A, IRAS 22340+2121, UGC 12103, MCG+03-57-021, PGC 69287[1]

NGC 7321 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 6,793±25 km/s, which corresponds to a Hubble distance of 326.8 ± 22.9 Mly (100.19 ± 7.02 Mpc).[1] However, seven non-redshift measurements give a closer mean distance of 297.50 ± 14.14 Mly (91.214 ± 4.334 Mpc).[2] It was discovered by German-British astronomer William Herschel on 17 November 1784.[3][4]

NGC 7321 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[5][6]

Galaxy group

According to M. J. Geller and J. P. Huchra, NGC 7321 is a member of a galaxy group which contains 2 other galaxies: NGC 7316 and NGC 7323 (fr).[7]

Supernovae

Two supernovae have been observed in NGC 7321:

See also

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "Results for object NGC 7321". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+7321. 
  2. ↑ 2.0 2.1 "Distance Results for NGC 7321". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+7321. 
  3. ↑ Herschel, William (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars". Philosophical Transactions of the Royal Society of London 76: 457–499. doi:10.1098/rstl.1786.0027. Bibcode: 1786RSPT...76..457H. https://zenodo.org/record/1432282/files/article.pdf. 
  4. ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 7321". https://cseligman.com/text/atlas/ngc73.htm#7321. 
  5. ↑ García-Lorenzo, B. et al. (2015). "Ionized gas kinematics of galaxies in the CALIFA survey. I. Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems". Astronomy and Astrophysics 573: A59. doi:10.1051/0004-6361/201423485. Bibcode: 2015A&A...573A..59G. 
  6. ↑ "NGC 7321". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+7321. 
  7. ↑ Geller, M. J.; Huchra, J. P. (1983). "Groups of galaxies. III. THe CfA survey". The Astrophysical Journal Supplement Series 52: 61. doi:10.1086/190859. Bibcode: 1983ApJS...52...61G. 
  8. ↑ Rex, J.; Li, W.; Cenko, S. B.; Filippenko, A. V. (2008). "Supernova 2008gj in NGC 7321". Central Bureau Electronic Telegrams (1541): 1. Bibcode: 2008CBET.1541....1R. http://www.cbat.eps.harvard.edu/iau/cbet/001500/CBET001541.txt. 
  9. ↑ "SN 2008gj". IAU. https://www.wis-tns.org/object/2008gj. 
  10. ↑ Howerton, S.; Drake, A. J.; Djorgovski, S. G.; Mahabal, A.; Graham, M. J.; Williams, R.; Prieto, J. L.; Catelan, M. et al. (2013). "Supernova 2013di in NGC 7321 = PSN J22362746+2136543". Central Bureau Electronic Telegrams (3562): 1. Bibcode: 2013CBET.3562....1H. 
  11. ↑ "SN 2013di". IAU. https://www.wis-tns.org/object/2013di. 

Coordinates: Sky map 22h 36m 28.0108s, +21° 37′ 18.648″