|Observation data (J2000 epoch)|
|Right ascension||00h 40m 31.3s|
|Declination||+40° 44′ 21″|
|Apparent dimensions (V)||4.2′|
|See also: Open cluster, List of open clusters|
NGC 206 is the richest and most conspicuous star cloud in M31 as well as one of the largest and brightest star formation regions of the Local Group. It contains more than 300 stars brighter than Mb=-3.6. It was originally identified by Edwin Hubble as a star cluster but today, due to its size, it is classified as an OB association.
NGC 206 is located in a spiral arm of the Andromeda Galaxy, in a zone free of neutral hydrogen and has a double structure, with one region that has an age of around 10 million years and includes several HII regions in one of its borders and other with an age of between 40 million years and 50 million years that includes a number of cepheids. Both parts are separated by a band of interstellar dust and include hundreds of stars of spectral type O and B.
- NGC 206 @ SEDS NGC objects pages
- NGC 206 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- "NASA/IPAC Extragalactic Database". Results for NGC 514. Retrieved 2006-11-25.
- Massey, Philip; Armandroff, Taft E.; Pyke, Randall; Patel, Kanan; Wilson, Christine D. (1995). "Hot, Luminous Stars in Selected Regions of NGC 6822, M31, and M33.". Astronomical Journal 110: 2715. Bibcode:1995AJ....110.2715M. doi:10.1086/117725.
- Hodge, Paul W. (1992). The Andromeda Galaxy. Springer. p. 153.
- Hodge, Paul W. (1992). The Andromeda Galaxy. Springer. p. 20. Retrieved 9 February 2012.
- Chernin, Arthur D.; Efremov, Yury N.; Voinovich, Peter A. (1995). "Superassociations: violent star formation induced by shock-shock collisions.". Monthly Notices of the Royal Astronomical Society 275 (2): 313–326. Bibcode:1995MNRAS.275..313C.
|This star cluster–related article is a stub. You can help Wikipedia by expanding it.|