OB star
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "OB_star".

OB stars are hot, massive stars of spectral types O or B which form in loosely organized groups called OB associations. They are short lived, and thus don't move very far from where they were formed within their life. During their lifetime, they will emit copious amounts of ultraviolet radiation. This radiation rapidly ionizes the surrounding interstellar gas of the giant molecular cloud, forming an H II region or Strömgren sphere.

In lists of spectra the "spectrum of OB" refers to "unknown, but belonging to an OB association so thus of early type".

References

• B. Cameron Reed (2003). "Catalog Of Galactic Ob Stars". The Astronomical Journal 125 (5): 2531 – 2533. doi:10.1086/374771, http://www.iop.org/EJ/article/1538-3881/125/5/2531/203021.html. 

See also

• Stellar association

External links

• [1] — Scientia Astrophysical Organization's star classification page

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