H II regions
type: Concept
definition: A type of emission nebulae composed of very hot gas (about 10^4 K), mainly ionized hydrogen, created by the ultraviolet radiation of massive stars. H II regions originate when O or early-type stars, born in giant molecular clouds, start heating up the cold gas, causing it to become ionized and 'glow'. The effective temperatures of the exciting stars are in the range 3 x 10^4 to 5 x 10^4 K, and throughout the nebula hydrogen is ionized. Helium is singly ionized, and other elements are mostly singly or doubly ionized. Typical densities in the H II region are of the order 10 to 10^2 cm^-3, ranging as high as 10^4 cm^-3. Internal motions occur in the gas with velocities of order 10 km s^-1. The spectra of H II regions are mainly composed of strong H I recombination lines and forbidden lines such as [O III], [O II], [N II].
alternative label: HII clouds
alternative label: H I I clouds
alternative label: H II clouds
alternative label: HII regions
alternative label: H I I regions
contributor: AAS Frey.Katie
contributor: AAS Frey.Katie Admin
modified: 2020-11-09T16:04:53.108Z
modified: 2020-11-02T15:59:55.394Z
narrower: Compact H II region
narrower: Bok globules
broader: Emission nebulae

Compact H II region
type: Concept
broader: H II regions

Bok globules
type: Concept
broader: H II regions

Emission nebulae
type: Concept
narrower: H II regions