Home  

Random  

Nearby  



Log in  



Settings  



Donate  



About Wikipedia  

Disclaimers  



Wikipedia





NGC 206





Article  

Talk  



Language  

Watch  

Edit  





NGC 206 is a bright star cloud in the Andromeda Galaxy, and the brightest star cloud in Andromeda when viewed from Earth.

NGC 206
NGC 206
Observation data (J2000 epoch)
Right ascension00h40m 31.3s[1]
Declination+40° 44′ 21″[1]
Apparent dimensions (V)4.2′ (arcmin)
Physical characteristics
RadiusCa. 400 ly
Associations
ConstellationAndromeda
See also: Open cluster, List of open clusters

Features

edit

NGC 206 is the richest and most conspicuous star cloud in the Andromeda Galaxy, and is one of the largest and brightest star-forming regions in the Local Group.[2] It contains more than 300 stars brighter than Mb=−3.6.[3] It was originally identified by Edwin Hubble as a star cluster but today, due to its size, it is classified as an OB association.[4]

NGC 206 is located in a spiral arm of the Andromeda Galaxy, in a zone free of neutral hydrogen. It contains hundreds of stars of spectral types O and B. The star cloud has a double structure: one region has an age of around 10 million years and includes several H II regions in its border; the other region has an age of 40 to 50 million years and includes a number of cepheids. The two regions are separated by a band of interstellar dust.[5]

See also

edit

References

edit
  1. ^ a b "NASA/IPAC Extragalactic Database". Results for NGC 206. Retrieved 25 November 2006.
  • ^ 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 Science & Business Media. p. 20. ISBN 978-0-7923-1654-1.
  • ^ 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. doi:10.1093/mnras/275.2.313.
  • edit


    Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_206&oldid=1190024748"




    Last edited on 15 December 2023, at 13:43  





    Languages

     


    العربية
    Asturianu
    Azərbaycanca
    Беларуская
    Bosanski
    Deutsch
    Ελληνικά
    Español
    Esperanto
    Euskara
    Français

    ि
    Hrvatski
    Italiano
    Қазақша
    Lëtzebuergesch
    Magyar
    Македонски

    Nederlands

    Нохчийн
    Oʻzbekcha / ўзбекча
    Polski
    Português
    Română
    Русский
    Slovenčina
    Српски / srpski
    Srpskohrvatski / српскохрватски
    Suomi
    Svenska
    Татарча / tatarça
    Türkçe
    Українська
    Tiếng Vit
    Zazaki

     

    Wikipedia


    This page was last edited on 15 December 2023, at 13:43 (UTC).

    Content is available under CC BY-SA 4.0 unless otherwise noted.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Terms of Use

    Desktop