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NGC 5806

Coordinates:Sky map15h 00m 00.4123s, +1° 53′ 28.756″
From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Virgo
NGC 5806
NGC 5806 imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationVirgo
Right ascension15h 00m 00.4123s[1]
Declination+01° 53′ 28.756″[1]
Redshift0.004493[1]
Heliocentric radial velocity1346 ± 21 km/s[2]
Distance68 Mly (21 Mpc)[3]
Group orclusterNGC 5806 Group (LGG 392)[4]
Apparent magnitude (V)11.70[3]
Apparent magnitude (B)12.40[3]
Characteristics
TypeSAB(s)b[1][3]
Size~73,900 ly (22.65 kpc) (estimated)[1]
Apparent size (V)3.1′ × 1.6′[3]
Other designations
IRAS 14574+0205,UGC 9645,MCG +00-38-014,PGC 53578,CGCG 020-041[2][1]

NGC 5806 is anintermediate spiral galaxy in theconstellationVirgo. It was discovered by German-British astronomerWilliam Herschel on 24 February 1786.[5] It is located about 70 millionlight-years (21Megaparsecs) away from the Milky Way.[3] It is a member of theNGC 5846 Group.[2]

Supernovae and Imposter

[edit]
Supernova SN 2004dg in NGC 5806

Threesupernovae and one supernova imposter have been observed in NGC 5806:

  • SN 2004dg (Type II, mag. 17.1) was discovered by Associazione Ternana Astrofili on 19 July 2004.[6][7] The progenitor of SN 2004dg has not been detected and is expected to have been a relatively low mass, low luminosity,red supergiant.[8]
  • SN 2012P (Type IIb, mag. 15.0) was discovered by Fabio Briganti on 22 January 2012.[9][10] Originally classified as aType Ib/c, it was later determined to be Type IIb.[11] Later analysis concluded that the progenitor had an initial mass of 15.2M.[12]
  • iPTF13bvn (Type Ib, mag. 17.2) was discovered by thePalomar Transient Factory on 16 June 2013.[13][14]
  • SN Hunt 248 (also known asAT 2014ib) was discovered by theCatalina Real-time Transient Survey and Stan Howerton on 21 May 2014. It was initially catalogued as a supernova, but was later classified as asupernova imposter. The progenitor was detected as a cool hypergiant with an absolute visual magnitude of −9 and 400,000 times more luminous than the sun. The eruption saw it increase in luminosity to around 80,000,000 L.[15] Later analysis concluded that this object is aluminous red nova.[16][17]

References

[edit]
  1. ^abcdef"Results for object NGC 5806".NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved2021-02-21.
  2. ^abc"NGC 5806".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-02-21.
  3. ^abcdefGil de Paz, Armando; et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies".The Astrophysical Journal Supplement Series.173 (2):185–255.arXiv:astro-ph/0606440.Bibcode:2007ApJS..173..185G.doi:10.1086/516636.S2CID 119085482.
  4. ^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.
  5. ^Seligman, Courtney."New General Catalogue objects: NGC 5800 - 5849".cseligman.com. Retrieved2021-02-21.
  6. ^Vagnozzi, A.; De Pasquale, D.; Guerri, F.; Guerri, G.; Cristofanelli, M.; Romanelli, S.; Valentini, S.; Yamaoka, H.; Itagaki, K. (July 2004)."Supernova 2004dg".International Astronomical Union Circular (8375). International Astronomical Union.Bibcode:2004IAUC.8375....1V.
  7. ^"SN 2004dg".Transient Name Server.IAU. Retrieved22 August 2024.
  8. ^Smartt, S. J.; Eldridge, J. J.; Crockett, R. M.; Maund, J. R. (2009)."The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae".Monthly Notices of the Royal Astronomical Society.395 (3): 1409.arXiv:0809.0403.Bibcode:2009MNRAS.395.1409S.doi:10.1111/j.1365-2966.2009.14506.x.S2CID 3228766.
  9. ^Dimai, A.; Briganti, F.; Brimacombe, J. (2012)."Supernova 2012P in NGC 5806 = PSN J14595904+0153251".Central Bureau Electronic Telegrams (2993): 1.Bibcode:2012CBET.2993....1D.
  10. ^"SN 2012P".Transient Name Server.IAU. Retrieved22 August 2024.
  11. ^Arcavi, Iair; Gal-Yam, Avishay; Ben-Ami, Sagi; Fox, Derek;Kasliwal, Mansi; Nugent, Peter; Howell, D. Andrew; Parrent, Jerod; Horesh, Assaf; Bellm, Eric; PTF Collaboration (2012)."PTF12os / PSN J14595904+0153251 is a Type IIb Supernova".The Astronomer's Telegram.3881: 1.Bibcode:2012ATel.3881....1A.
  12. ^Sun, Ning-Chen; Maund, Justyn R.; Crowther, Paul A.; Fang, Xuan; Zapartas, Emmanouil (2021)."Towards a better understanding of supernova environments: A study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE".Monthly Notices of the Royal Astronomical Society.504 (2): 2253.arXiv:2011.13667.Bibcode:2021MNRAS.504.2253S.doi:10.1093/mnras/stab994.
  13. ^Cao, Y.; Gorbikov, E.; Arcavi, I.; Ofek, E.; Gal-Yam, A.; Nugent, P.;Kasliwal, M. (2013)."IPTF discovery of a young SN candidate at z=0.00449".The Astronomer's Telegram.5137: 1.Bibcode:2013ATel.5137....1C.
  14. ^Fremling, C.; Sollerman, J.; Taddia, F.; Ergon, M.; Fraser, M.; Karamehmetoglu, E.; Valenti, S.; Jerkstrand, A.; Arcavi, I.; Bufano, F.; Elias Rosa, N.; Filippenko, A. V.; Fox, D.; Gal-Yam, A.; Howell, D. A.; Kotak, R.; Mazzali, P.; Milisavljevic, D.; Nugent, P. E.; Nyholm, A.; Pian, E.; Smartt, S. (2016). "PTF12os and iPTF13bvn".Astronomy & Astrophysics.593: A68.arXiv:1606.03074.doi:10.1051/0004-6361/201628275.S2CID 54028503.
  15. ^Mauerhan, Jon C.; Van Dyk, Schuyler D.; Graham, Melissa L.; Zheng, Weikang; Clubb, Kelsey I.; Filippenko, Alexei V.; Valenti, Stefano; Brown, Peter; Smith, Nathan; Howell, D. Andrew; Arcavi, Iair (2015)."SN Hunt 248: A super-Eddington outburst from a massive cool hypergiant".Monthly Notices of the Royal Astronomical Society.447 (2): 1922.arXiv:1407.4681.Bibcode:2015MNRAS.447.1922M.doi:10.1093/mnras/stu2541.S2CID 11415725.
  16. ^"Classification certificate for object 2014ib".Transient Name Server.IAU. Retrieved5 June 2025.
  17. ^Mauerhan, Jon C.; Van Dyk, Schuyler D.; Johansson, Joel; Fox, Ori D.; Filippenko, Alexei V.; Graham, Melissa L. (2018)."The dusty aftermath of SN Hunt 248: Merger-burst remnant?".Monthly Notices of the Royal Astronomical Society.473 (3): 3765.arXiv:1702.00430.Bibcode:2018MNRAS.473.3765M.doi:10.1093/mnras/stx2500.

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