NGC 759

NGC 759
2MASS image of NGC 759.
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension01h 57m 50.3s[1]
Declination36° 20′ 35″[1]
Redshift0.015567[1]
Heliocentric radial velocity4667 km/s[1]
Distance230 Mly (70.4 Mpc)[1]
Group or clusterAbell 262
Apparent magnitude (V)13.3[1]
Characteristics
TypeE[1]
Size~110,000 ly (33 kpc) (estimated)[1]
Apparent size (V)1.6 × 1.4[1]
Other designations
MCG 6-5-67, PGC 7397, UGC 1440[1]
Preview warning: Page using Template:Infobox galaxy with unknown parameter "upright"

NGC 759 is an elliptical galaxy located 230 million light-years away[2] in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865.[3] It is a member of Abell 262.[4][5][6][7][8]

Despite being classified as a radio galaxy,[9][10][11][12][13] the radio emission in NGC 759 could be due to star formation rather than an active galactic nucleus.[12][13]

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 759. Retrieved 2019-01-06.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-01-08.
  3. ^ "New General Catalog Objects: NGC 750 – 799". cseligman.com. Retrieved 2019-01-03.
  4. ^ Giuricin, G.; Marinoni, C.; Ceriani, L.; Pisani, A. (November 2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN 0004-637X. S2CID 9618325.
  5. ^ Garcia, A. M. (1993-07-01). "General study of group membership. II – Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
  6. ^ Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992-05-01). "Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211–233. Bibcode:1992A&AS...93..211F. ISSN 0365-0138.
  7. ^ "NGC 759". simbad. Retrieved 2019-01-08.
  8. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-01-08.
  9. ^ Righetti, G.; Giovannini, G.; Feretti, L. (1988-04-01). "WSRT observations at 327 MHz of the cluster A262". Astronomy and Astrophysics Supplement Series. 73: 173–179. Bibcode:1988A&AS...73..173R. ISSN 0365-0138.
  10. ^ Zhao, Jun-Hui; Burns, Jack O.; Owen, Frazer N. (1989-07-01). "A 20 CM VLA survey of Abell clusters of galaxies. I – Distance class of not greater than 3 clusters". The Astronomical Journal. 98: 64–107. Bibcode:1989AJ.....98...64Z. doi:10.1086/115128. ISSN 0004-6256.
  11. ^ Miller, Neal A.; Owen, Frazer N. (2001-06-01). "The Radio Galaxy Populations of Nearby Northern Abell Clusters". The Astrophysical Journal Supplement Series. 134 (2): 355–383. arXiv:astro-ph/0101114. Bibcode:2001ApJS..134..355M. doi:10.1086/320857. ISSN 0067-0049. S2CID 119052072.
  12. ^ a b Feretti, L.; Giovannini, G. (1994-01-01). "Structures of small-size radio galaxies in clusters". Astronomy and Astrophysics. 281: 375–387. Bibcode:1994A&A...281..375F. ISSN 0004-6361.
  13. ^ a b Vila-Vilaró, B.; Cepa, J.; Butner, H. M. (2003-09-01). "CO (3–2) Observations of Early-Type Galaxies with the Heinrich Hertz Telescope". The Astrophysical Journal. 594 (1): 232–246. Bibcode:2003ApJ...594..232V. doi:10.1086/376775. ISSN 0004-637X.