NGC 703

In today's world, NGC 703 has become a topic of great interest and relevance in different areas. The growing importance of NGC 703 has sparked a debate in society, generating growing interest in understanding its implications. From diverse perspectives, NGC 703 has become an object of study and research, giving rise to numerous analyzes and reflections that seek to understand its impact and scope. In this article, we will explore the different facets of NGC 703, examining its influence in different contexts and its role in contemporary society.

NGC 703
Pan-STARRS image of NGC 703
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension01h 52m 39.6s[1]
Declination36° 10′ 17″[1]
Redshift0.018613[1]
Heliocentric radial velocity5580 km/s[1]
Distance240 Mly (73 Mpc)[1]
Group or clusterAbell 262
Apparent magnitude (V)14.27[1]
Characteristics
TypeS0^-[1]
Size~82,000 ly (25 kpc) (estimated)[1]
Apparent size (V)1.2 x 0.9[1]
Other designations
CGCG 522-37, MCG 6-5-29, PGC 6957, UGC 1346[1]

NGC 703 is a lenticular galaxy located 240 million light-years away[2] in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786[3] and is also a member of Abell 262.[4][5][6][7]

NGC 703 is classified as a radio galaxy.[8][9][10][11]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 703. Retrieved 2018-11-23.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-11-23.
  3. ^ "New General Catalog Objects: NGC 700 – 749". cseligman.com. Retrieved 2018-11-21.
  4. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-11-23.
  5. ^ M., Garcia, A. (July 1993). "General study of group membership. II – Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  6. ^ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN 0004-637X. S2CID 9618325.
  7. ^ Reddy, Naveen A.; Yun, Min S. (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.
  8. ^ "NGC 703". sim-id. Retrieved 2018-12-24.
  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. ^ Blanton, Elizabeth L.; Sarazin, Craig L.; McNamara, Brian R.; Clarke, T. E. (2004-09-10). "Chandra Observation of the Central Region of the Cooling Flow Cluster Abell 262: A Radio Source that is a Shadow of its Former Self?". The Astrophysical Journal. 612 (2): 817–824. arXiv:astro-ph/0405425. Bibcode:2004ApJ...612..817B. doi:10.1086/422677. ISSN 0004-637X. S2CID 2628446.
  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.