NGC 6047

NGC 6047 is an elliptical galaxy located about 430 million light-years away[2] in the constellation Hercules.[3] It was discovered by astronomer Lewis Swift on June 27, 1886.[4] NGC 6047 is a member of the Hercules Cluster.[5][6][7]

NGC 6047
SDSS image of NGC 6047.
Observation data (J2000 epoch)
ConstellationHercules
Right ascension16h 05m 09.0s[1]
Declination17° 43′ 48″[1]
Redshift0.031262[1]
Helio radial velocity9372 km/s[1]
Distance131.4 Mpc (429 Mly)[1]
Group or clusterHercules Cluster
Apparent magnitude (V)14.55[1]
Characteristics
TypeE+, cD[1]
Size~170,000 ly (52 kpc)[1] (estimated)[1]
Apparent size (V)1.1 x 0.8[1]
Notable featuresradio jet
Other designations
CGCG 108-111, DRCG 34-62, 4C +17.66, PKS 1602+178, MCG+3-41-87, PGC 57033[1]

Morphology

NGC 6047 has a peculiar morphology[5][8][9]which suggests it has undergone a recent merger.[6][7][10]

Radio jets

NGC 6047 has two radio jets[6][7] and is classified as a FR I radio galaxy.[9]

The jets appear to have a Z-shaped structure.[5]

Interaction with NGC 6045

NGC 6047 may be interacting with NGC 6045 which lies around ~320,000 ly (97 kpc) away.[8]

See also

References
  1. "NASA/IPAC Extragalactic Database". Results for NGC 6047. Retrieved 2018-08-16.
  2. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-08-20.
  3. "Revised NGC Data for NGC 6047". spider.seds.org. Retrieved 2018-08-21.
  4. "New General Catalog Objects: NGC 6000 - 6049". cseligman.com. Retrieved 2018-08-21.
  5. Feretti, L.; Giovannini, G. (February 1988). "NGC 6047 - Radio source interaction with the environment". Astronomy and Astrophysics. 191: 21. Bibcode:1988A&A...191...21F. ISSN 0004-6361.
  6. Liuzzo, E.; Giovannini, G.; Giroletti, M.; Taylor, G. B. (June 2010). "Parsec-scale properties of brightest cluster galaxies". Astronomy and Astrophysics. 516: A1. arXiv:1002.1380. Bibcode:2010A&A...516A...1L. doi:10.1051/0004-6361/200913888. ISSN 0004-6361. S2CID 14536396.
  7. Liuzzo, E.; Giovannini, G.; Giroletti, M. (March 2011). "Nuclear properties of Brightest Cluster Galaxies: results and new observations for two peculiar cases". arXiv:1103.0450 [astro-ph.CO].
  8. 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.
  9. Heckman, T. M.; Smith, Eric P.; Baum, Stefi A.; van Breugel, W. J. M.; Miley, G. K.; Illingworth, G. D.; Bothun, G. D.; Balick, B. (December 15, 1986). "Galaxy collisions and mergers - The genesis of very powerful radio sources?". The Astrophysical Journal. 311: 526–547. Bibcode:1986ApJ...311..526H. doi:10.1086/164793. ISSN 0004-637X.
  10. Dickey, John M. (June 1997). "A VLA Survey of the Hercules Cluster.I.The HI Data". The Astronomical Journal. 113: 1939. Bibcode:1997AJ....113.1939D. doi:10.1086/118408. ISSN 0004-6256.


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