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NGC 4567 and NGC 4568

From Wikipedia, the free encyclopedia
Interacting galaxy pair in the constellation Virgo
NGC 4567 and NGC 4568
The Butterfly Galaxies with NGC 4567 (top) and NGC 4568 (bottom)
Observation data (J2000.0epoch)
ConstellationVirgo
Right ascension12h 36m 34.3s
Declination+11° 14′ 17″
Distance62 Mly (19.1 Mpc)[1]
Apparent magnitude (V)+10.9
Absolute magnitude (V)-13.3
Characteristics
TypeSA(rs)bc / SA(rs)bc
Apparent size (V)4.6′ × 2.1′
Notable featurescolliding galaxies
Other designations
NGC 4567/8,UGC 7776/7,PGC 42064/9,VV 219,[2] KPG 347,[3] Butterfly Galaxies,[4] Siamese Twin Galaxies, Siamese Twins Galaxies, Siamese Twins[5][NB 1]

NGC 4567 and NGC 4568 (nicknamed theButterfly Galaxies[4] orSiamese Twins[NB 1][5]) are a set ofunbarred spiral galaxies about 60 millionlight-years away[1] in theconstellationVirgo. They were both discovered byWilliam Herschel in 1784. They are part of theVirgo Cluster ofgalaxies.

These galaxies are in the process ofcolliding and merging with each other, as studies of their distributions ofneutral and molecularhydrogen show, with the higheststar-formation activity in the part where they overlap. However, the system is still in an early phase of interaction.[6] In about 500 million years the galaxies will coalesce into a single elliptical galaxy.[7]

Supernovae

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SN 2020fqv shown in NGC 4568

Foursupernovae have been observed in the Butterfly Galaxies:

SN 2023idj in NGC 4568 as seen on 2023-May-17.

Naming controversy

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The two galaxies were nicknamed "Siamese Twins" because they appear to be connected. On August 5, 2020, NASA announced that they would not use that nickname in an effort to avoidsystemic discrimination in their terminology.[14][15]

See also

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Notes

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  1. ^abNASA no longer uses the "Siamese Twins" terms due to perceived discriminatory naming

References

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  1. ^ab"Distance Results for NGC 4568".NASA/IPAC Extragalactic Database. Retrieved2010-05-01.
  2. ^"VV 219 -- Interacting Galaxies". SIMBAD.
  3. ^"KPG 347 -- Pair of Galaxies". SIMBAD.
  4. ^abXu, Cong; Gao, Yu; Mazzarella, Joseph; Lu, Nanyao; Sulentic, Jack W.; Domingue, Donovan L. (2000). "Mapping Infrared Enhancements in Closely Interacting Spiral-Spiral Pairs. I.ISO CAM andISO SWS Observations".The Astrophysical Journal.541 (2):644–659.arXiv:astro-ph/0005025.Bibcode:2000ApJ...541..644X.doi:10.1086/309483.
  5. ^abCudnik B. (2013). "The Nature of Galaxies and Galaxy Clusters".Faint Objects and How to Observe Them. Astronomers' Observing Guides. Springer. pp. 71–91.doi:10.1007/978-1-4419-6757-2_4.ISBN 978-1-4419-6756-5.
  6. ^Kaneko, H.; Kuno, N.; Iono, D.; Tosaki, T.; Sawada, T.; Nakanishi, H.; Hirota, A. (2010). "Molecular Gas in the Early Stage of Interacting Galaxies: The NGC 4567/8 Pair".Galaxy Wars: Stellar Populations and Star Formation in Interacting Galaxies.423: 26.Bibcode:2010ASPC..423...26K.
  7. ^"The merging galaxy pair NGC 4568 and NGC 4567".
  8. ^Perlmutter, S.; Pennypacker, C. (1990)."Supernova 1990B in NGC 4568".International Astronomical Union Circular (4949): 1.Bibcode:1990IAUC.4949....1P.
  9. ^"SN 1990B".Transient Name Server.IAU. Retrieved6 December 2024.
  10. ^Monard, L. A. G.; Li, W. (2004)."Supernovae 2004bz, 2004ca, 2004cb, 2004cc".International Astronomical Union Circular (8350): 2.Bibcode:2004IAUC.8350....2M.
  11. ^"SN 2004cc".Transient Name Server.IAU. Retrieved6 December 2024.
  12. ^"SN 2020fqv".Transient Name Server.IAU. Retrieved6 December 2024.
  13. ^"SN 2023ijd".Transient Name Server.IAU. Retrieved6 December 2024.
  14. ^Haworth, Jon (August 9, 2020),"NASA drops 'insensitive' celestial nicknames in effort to address systemic discrimination",ABC News, retrieved2020-08-10
  15. ^"NASA to Reexamine Nicknames for Cosmic Objects - NASA". 5 August 2020.

External links

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Wikimedia Commons has media related toNGC 4567.
Wikimedia Commons has media related toNGC 4568.
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