: Astronomy: H II region

interstellar space > interstellar matter > nebula > emission nebula > H II region

H II region

An HII region is a volume of space where the hydrogen in the interstellar medium is in an ionized rather than a neutral state. Generally, HII regions occur where hot, blue OB stars are pouring large amounts of ultraviolet radiation into the surrounding cloud from which they were recently formed. Such stars can ionize all the hydrogen (and other atoms) for dozens or even hundreds of light-years in every direction. The ultraviolet light strips electrons away from hydrogen atoms by the process known as photoionization. Then as the electrons recombine with protons (hydrogen nuclei) they emit a characteristic series of emission lines as they cascade down through the energy levels of the atom. The visible radiation in these lines imparts to HII regions their beautiful colored glows. (Encyclopedia of Science, by David Darling, https://www.daviddarling.info/encyclopedia/H/HII.html)

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