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Concept information

Preferred term

H I region  

Definition(s)

  • An HI region is an interstellar cloud composed primarily of atomic hydrogen, detectable by its radio wave emission in the 21-centimeter line. HI regions have a density of 1 to 10 atoms/cm3 and a temperature of about 125 K (the spin temperature of neutral hydrogen). At least 95% of interstellar hydrogen is HI. (Encyclopedia of Science, by David Darling, https://www.daviddarling.info/encyclopedia/H/HI.html)

Broader concept(s)

Synonym(s)

  • H1 region
  • H I cloud
  • HI region

In other languages

URI

http://data.loterre.fr/ark:/67375/MDL-J8K8RTSN-L

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