Misplaced Pages

NGC 2442 and NGC 2443

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Spiral galaxy in the constellation Volans
NGC 2442 / 2443
NGC 2442 (upper spiral structure) and NGC 2443 (lower horizontal spiral arm)
Observation data (J2000 epoch)
ConstellationVolans
Right ascension07 36 23.8
Declination−69° 31′ 51″
Redshift1466 ± 5 km/s
Apparent magnitude (V)11.2
Characteristics
TypeSAB(s)bc pec
Apparent size (V)5′.5 × 4′.9
Notable featuresSW part is NGC 2442
while NE part is NGC 2443
Other designations
PGC 21373

NGC 2442 and NGC 2443 are two parts of a single intermediate spiral galaxy, commonly known as the Meathook Galaxy or the Cobra and Mouse. It is about 50 million light-years away in the constellation Volans. It was discovered by Sir John Herschel on December 23, 1834 during his survey of southern skies with a 18.25 inch diameter reflecting telescope (his "20-foot telescope") from an observatory he set up in Cape Town, South Africa. Associated with this galaxy is HIPASS J0731-69, a cloud of gas devoid of any stars. It is likely that the cloud was torn loose from NGC 2442 by a companion.

When John Louis Emil Dreyer compiled the New General Catalogue of Nebulae and Clusters of Stars he used William Herschel's earlier observations that described two objects in a "double nebula", giving the northern most the designation NGC 2443 and the southernmost most the designation NGC 2442. Herschel's later observations noted that the two objects were actually a single large nebula.

Supernovae

Two, or perhaps three, supernovae have been observed in NGC 2442:

  • SN 1999ga (type II, mag. 18) was discovered by the Perth Astronomical Research Group on 19 November 1999.
  • SN 2015F (type Ia, mag. 16.8) was discovered by Libert "Berto" Monard on 9 March 2015. It reached magnitude 12.9, making it the brightest supernova of 2015.
  • Gaia16cfr, also known as AT 2016jbu, was a supernova imposter that occurred in NGC 2442 on 1 December 2016. It reached a Gaia apparent magnitude of 19.3 and absolute magnitude of about −12. However, a paper published in August 2022 suggested that this was a genuine, but strange, supernova.

References

  1. NGC/IC Project Restoration Effortngcicproject.observers.org
  2. ^ "NASA/IPAC Extragalactic Database". Results for NGC 2442 / 2443. Retrieved 2023-02-08.
  3. Chadwick, S; Cooper, I (11 December 2012). Imaging the Southern Sky. New York: Springer. p. 263. ISBN 978-1461447498.
  4. ^ Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 2400 - 2449". cseligman.com. Archived from the original on 9 September 2015. Retrieved 10 July 2015.
  5. ^ Ryder, S.D.; et al. (July 2001). "HIPASS Detection of an Intergalactic Gas Cloud in the NGC 2442 Group". The Astrophysical Journal. 555 (1): 232–239. arXiv:astro-ph/0103099. Bibcode:2001ApJ...555..232R. doi:10.1086/321453. S2CID 14455875.
  6. NGC/IC Project Restoration Effortngcicproject.observers.org
  7. Woodings, S.; Martin, R.; Williams, A.; Biggs, J.; Verveer, A. (1999). "Supernova 1999ga in NGC 2442". International Astronomical Union Circular (7316): 1. Bibcode:1999IAUC.7316....1W.
  8. "SN 1999ga". Transient Name Server. IAU. Retrieved 9 December 2024.
  9. Monard, L. A. G.; Fraser, M.; Smith, M.; Firth, R.; Dimitriadis, G.; Frohmaier, C.; Cartier, R.; Prajs, S.; Sullivan, M.; Anderson, J.; Maguire, K.; Inserra, C.; Smartt, S. J.; Smith, K. W.; Young, D.; Valenti, S.; Yaron, O.; Manulis, I. (2015). "Supernova 2015F in NGC 2442 = PSN J07361576-6930230". Central Bureau Electronic Telegrams. 4081: 1. Bibcode:2015CBET.4081....1M.
  10. "SN 2015F". Transient Name Server. IAU. Retrieved 9 December 2024.
  11. Bishop, David. "Bright Supernovae - 2015". Rochester Astronomy. Retrieved 9 December 2024.
  12. "AT 2016jbu". Transient Name Server. IAU. Retrieved 31 August 2024.
  13. Fox, Derek (4 January 2017). "PESSTO classification and characterisation of AT 2016jbu / Gaia16cfr". The Astronomer's Telegram. Retrieved 31 August 2024.
  14. Kilpatrick, Charles D.; Foley, Ryan J.; Drout, Maria R.; Pan, Yen-Chen; Panther, Fiona H.; Coulter, David A.; Filippenko, Alexei V.; Marion, G. Howard; Piro, Anthony L.; Rest, Armin; Seitenzahl, Ivo R.; Strampelli, Giovanni; Wang, Xi E. (2018). "Connecting the progenitors, pre-explosion variability and giant outbursts of luminous blue variables with Gaia16cfr". Monthly Notices of the Royal Astronomical Society. 473 (4): 4805. arXiv:1706.09962. Bibcode:2018MNRAS.473.4805K. doi:10.1093/mnras/stx2675.
  15. Brennan, S. J.; Elias-Rosa, N.; Fraser, M.; Van Dyk, S. D.; Lyman, J. D. (2022). "The impostor revealed: SN 2016jbu was a terminal explosion". Astronomy and Astrophysics. 664: L18. arXiv:2206.06365. Bibcode:2022A&A...664L..18B. doi:10.1051/0004-6361/202244262.

External links


Astronomical catalogs
NGC
PGC
New General Catalogue 2000 to 2499
Constellation of Volans
Stars
Bayer
Variable
HR
HD
Other
Exoplanets
Galaxies
NGC
Other
Galaxy clusters
Category


Stub icon

This spiral galaxy article is a stub. You can help Misplaced Pages by expanding it.

Categories: