 |
This article relies largely or entirely on a single source. Relevant discussion may be found on the talk page. Please help improve this articlebyintroducing citations to additional sources.
Find sources: "OB star" – news · newspapers · books · scholar · JSTOR (June 2016) |
OB stars are hot, massive stars of spectral types Oorearly-type B that form in loosely organized groups called OB associations. They are short lived, and thus do not move very far from where they formed within their life. During their lifetime, they will emit much ultraviolet radiation. This radiation rapidly ionizes the surrounding interstellar gas of the giant molecular cloud, forming an H II regionorStrömgren sphere.
In lists of spectra the "spectrum of OB" refers to "unknown, but belonging to an OB association so thus of early type".[dubious – discuss]
|
| |||||||
|---|---|---|---|---|---|---|---|
| |||||||
| Formation |
| ||||||
| Evolution |
| ||||||
| Classification |
| ||||||
| Nucleosynthesis |
| ||||||
| Structure |
| ||||||
| Properties |
| ||||||
| Star systems |
| ||||||
| Earth-centric observations |
| ||||||
| Lists |
| ||||||
| Related |
| ||||||
| |||||||
 | This article about stellar astronomy is a stub. You can help Wikipedia by expanding it. |
