Astronomy:NGC 7316

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NGC 7316
NGC 7316 imaged by SDSS
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension 22h 35m 56.3485s[1]
Declination+20° 19′ 19.666″[1]
Redshift0.018529±0.00000200[1]
Helio radial velocity5,555±1 km/s[1]
Distance212.87 ± 3.89 Mly (65.267 ± 1.192 Mpc)[2]
Apparent magnitude (V)13.62[1]
Characteristics
TypeSBc[1]
Size~77,800 ly (23.86 kpc) (estimated)[1]
Apparent size (V)1.1′ × 0.9′[1]
Other designations
IRAS 22335+2003, UGC 12098, MCG+03-57-020, PGC 69259[1]

NGC 7316 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 5,198±25 km/s, which corresponds to a Hubble distance of 250.1 ± 17.5 Mly (76.67 ± 5.38 Mpc).[1] However, three non-redshift measurements give a closer mean distance of 212.87 ± 3.89 Mly (65.267 ± 1.192 Mpc).[2] It was discovered by German-British astronomer William Herschel on 18 September 1784.[3][4]

NGC 7316 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[5][6] NGC 7316 is also a starburst galaxy.[1]

NGC 7316 has a nucleus with excessive amounts of ultraviolet emissions compared with other galaxies, and is listed in the Markarian catalogue as MRK 307.[7]

Galaxy group

According to M. J. Geller and J. P. Huchra, NGC 7316 is a member of a galaxy group which contains 2 other galaxies: NGC 7321 and NGC 7323 (fr).[8]

Supernovae

Two supernovae have been observed in NGC 7316:

See also

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "Results for object NGC 7316". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+7316. 
  2. ↑ 2.0 2.1 "Distance Results for NGC 7316". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+7316. 
  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 7316". https://cseligman.com/text/atlas/ngc73.htm#7316. 
  5. ↑ Asmus, D.; Greenwell, C. L.; Gandhi, P.; Boorman, P. G.; Aird, J.; Alexander, D. M.; Assef, R. J.; Baldi, R. D. et al. (2020). "Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 MPC". Monthly Notices of the Royal Astronomical Society 494 (2): 1784. doi:10.1093/mnras/staa766. Bibcode: 2020MNRAS.494.1784A. 
  6. ↑ "NGC 7316". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+7316. 
  7. ↑ Markaryan, B. E.; Lipovetskii, V. A. (1971). "Galaxies with an ultraviolet continuum. IV". Astrophysics 7 (4): 299. doi:10.1007/BF01003012. Bibcode: 1971Ap......7..299M. 
  8. ↑ 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. 
  9. ↑ Prasad, R. R.; Li, W. (2006). "Supernova 2006cx in NGC 7316". Central Bureau Electronic Telegrams (542): 1. Bibcode: 2006CBET..542....1P. http://www.cbat.eps.harvard.edu/iau/cbet/000500/CBET000542.txt. 
  10. ↑ "SN 2006cx". IAU. https://www.wis-tns.org/object/2006cx. 
  11. ↑ Zhang, Jujia; Xin, Yuxin; Xiang, Danfeng; Rui, Liming; Wang, Xiaofeng; Cao, Tianwen; Wang, Huijuan; Zhang, Tianmeng (2016). "Spectroscopic Classification of SN 2016hvu as a Young Type IIP Supernova". The Astronomer's Telegram 9746: 1. Bibcode: 2016ATel.9746....1Z. https://www.astronomerstelegram.org/?read=9746. 
  12. ↑ "SN 2016hvu". IAU. https://www.wis-tns.org/object/2016hvu. 

Coordinates: Sky map 22h 35m 56.3485s, +20° 19′ 19.666″



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