The nature of the galactic H I supershells

Details The nature of the galactic H I supershells The nature of the galactic H I supershells

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..214g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Apr. 1982, p. 214-218.) Soviet Astronomy Letters, vol. 8, Mar.-Apr. 1982, p. 113-115

Astronomy and Astrophysics

Astronomy

7

Galactic Structure, Hydrogen Clouds, Mass Distribution, Milky Way Galaxy, Neutral Gases, Galactic Rotation, Line Spectra, Radio Spectra

Scientific paper

It is suggested that the majority of the shell and supershell formations typical of neutral hydrogen's galactic distribution reflect a normal, stratified spiral structure rather than structures produced by the impacts of supernova remnants or stellar wind on the interstellar medium. If this interpretation is correct, the observed profiles of the H I radio line from the shells would be determined by differential galactic rotation.

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