NGC 6045 is a barred spiral galaxy located about 450 million light-years away[2] in the constellation Hercules.[3] NGC 6045 was discovered by astronomer Lewis Swift on June 27, 1886[4] and is a member of the Hercules Cluster.[5][4] It is also a LINER galaxy.[6]

NGC 6045
Sloan Digital Sky Survey image of NGC 6045. The small, nearby galaxy at left portion of the image is PGC 84720.
Observation data (J2000 epoch)
ConstellationHercules
Right ascension16h 05m 07.9s[1]
Declination17° 45′ 28″[1]
Redshift0.033310[1]
Heliocentric radial velocity9986 km/s[1]
Distance137 Mpc (447 Mly)[1]
Group or clusterHercules Cluster
Apparent magnitude (V)14.9[1]
Characteristics
TypeSB(s)c[1]
Size~183,300 ly (56.20 kpc)[1] (estimated)[1]
Apparent size (V)1.17 x 0.28[1]
Notable featuresWarped disk
Other designations
PGC 057031, UGC 10177, Arp 71, MCG +03-41-088[1]

Possible interaction

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NGC 6045 is very luminous in both X-ray[5] and infrared light.[7] This high luminosity in both X-ray and infrared has been suggested to be the result of a starburst event in the galaxy.[5][7] It is thought that starburst events are caused by interactions or mergers with other galaxies.[8][5] Also, NGC 6045 has a warped disk which may be due to an interaction[7] with the elliptical galaxy NGC 6047 which lies around ~320,000 ly (97 kpc) from the galaxy.[5]

See also

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References

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  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 6045. Retrieved 2018-02-01.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-02-02.
  3. ^ "Revised NGC Data for NGC 6045". spider.seds.org. Retrieved 2018-02-02.
  4. ^ a b "New General Catalog Objects: NGC 6000 - 6049". cseligman.com. Retrieved 2018-01-25.
  5. ^ a b c d e Huang, Zhenping; Sarazin, Craig L. (April 1996). "A High-Resolution ROSAT X-Ray Study of the Hercules Cluster". The Astrophysical Journal. 461: 622. Bibcode:1996ApJ...461..622H. doi:10.1086/177090. ISSN 0004-637X.
  6. ^ "NGC 6045". Retrieved 2018-08-17.
  7. ^ a b c Young, E.; Low, F. J.; Soifer, B. T.; Neugebauer, G.; Rowan-Robinson, M.; Clegg, P. E.; Miley, G.; de Jong, T.; Gautier, T. N. (March 1984). "The infrared properties of galaxy clusters - IRAS observations of the Hercules Cluster (Abell 2151)". The Astrophysical Journal. 278: L75–L78. Bibcode:1984ApJ...278L..75Y. doi:10.1086/184227. hdl:1887/6462. ISSN 0004-637X.
  8. ^ "Chandra :: Field Guide to X-ray Sources :: Starburst Galaxies". chandra.harvard.edu. Retrieved 2018-02-03.
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