NGC 710

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NGC 710
NGC 710 PanS.jpg
NGC 710 imaged by Pan-STARRS
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 52m 53.9666s [1]
Declination +36° 03′ 10.162″ [1]
Redshift 0.020431 [1]
Heliocentric radial velocity 6125 ± 7 km/s [1]
Distance 282.5 ± 19.8  Mly (86.60 ± 6.07  Mpc) [1]
Group or cluster Abell 262
Apparent magnitude  (V)14.27 [1]
Characteristics
Type Scd [1]
Size~57,600  ly (17.65  kpc) (estimated) [1]
Apparent size  (V)1.3′ × 1.2′ [1]
Other designations
IRAS 01499+3548, UGC 1349, MCG +06-05-033, PGC 6972, CGCG 522-041 [1]

NGC 710 is a spiral galaxy located 260 million light-years away [2] in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 [3] [4] and is a member of the galaxy cluster Abell 262. [5] [6] [7] [8] [9]

Contents

It is also a radio galaxy. [10] [11] [12] [13]

Supernovae

Two supernovae have been observed in NGC 710:

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 0710". NASA/IPAC Extragalactic Database. Retrieved 2018-12-26.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-27.
  3. ↑ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
  4. ↑ Seligman, Courtney. "The Discoverers of the NGC / IC Objects". Celestial Atlas. Retrieved 28 December 2018.
  5. ↑ "NGC 710". sim-id. Retrieved 2018-12-27.
  6. ↑ Steinicke, Wolfgang (2010-08-19). Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. p. 309. ISBN   978-1-139-49010-8.
  7. ↑ Scodeggio, Marco; Boselli, Alessandro; Gavazzi, Giuseppe; Trinchieri, Ginevra; Garilli, Bianca (1992-08-01). "Multifrequency windows on spiral galaxies. II - The A262 and Cancer clusters". Astronomy and Astrophysics Supplement Series. 94: 299–326. Bibcode:1992A&AS...94..299S. ISSN   0365-0138.
  8. ↑ Butcher, H. R.; Oemler, A. Jr. (1985-04-01). "The evolution of galaxies in clusters. IV - Photometry of 10 low-redshift clusters". The Astrophysical Journal Supplement Series. 57: 665–691. Bibcode:1985ApJS...57..665B. doi:10.1086/191022. ISSN   0067-0049.
  9. ↑ Fanti, C.; Fanti, R.; Feretti, L.; Ficarra, A.; Gioia, I. M.; Giovannini, G.; Gregorini, L.; Mantovani, F.; Marano, B. (1982-01-01). "Radio and optical observations of 9 nearby Abell clusters - A262, A347, A569, A576, A779, A1213, A1228, A2162, A2666". Astronomy and Astrophysics. 105: 200–218. Bibcode:1982A&A...105..200F. ISSN   0004-6361.
  10. ↑ Yun, Min S.; Reddy, Naveen A. (January 10, 2004). "Radio and Far-Infrared Emission as Tracers of Star Formation and Active Galactic Nuclei in Nearby Cluster Galaxies". The Astrophysical Journal. 600 (2): 695–715. arXiv: astro-ph/0309649 . Bibcode:2004ApJ...600..695R. doi:10.1086/379871. ISSN   0004-637X. S2CID   15068448.
  11. ↑ Miller, Neal A.; Owen, Frazer N. (2001). "The Radio Galaxy Populations of Nearby Northern Abell Clusters". The Astrophysical Journal Supplement Series. 134 (2): 355–384. arXiv: astro-ph/0101114 . Bibcode:2001ApJS..134..355M. doi:10.1086/320857. ISSN   0067-0049. S2CID   119052072.
  12. ↑ 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.
  13. ↑ Fanti, C.; Fanti, R.; Feretti, L.; Ficarra, A.; Gioia, I. M.; Giovannini, G.; Gregorini, L.; Mantovani, F.; Marano, B. (1982-01-01). "Radio and optical observations of 9 nearby Abell clusters - A262, A347, A569, A576, A779, A1213, A1228, A2162, A2666". Astronomy and Astrophysics. 105: 200–218. Bibcode:1982A&A...105..200F. ISSN   0004-6361.
  14. ↑ Li, W. D. (1 August 2002). "Supernova 2002eo in NGC 710". International Astronomical Union Circular. 7958: 1. Bibcode:2002IAUC.7958....1L.
  15. ↑ "Bright Supernovae - 2002". rochesterastronomy.org. Retrieved 2018-12-27.
  16. ↑ "SN 2002eo". Transient Name Server. IAU . Retrieved 20 October 2025.
  17. ↑ "SN 2025zmx". Transient Name Server. IAU . Retrieved 20 October 2025.
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