Nature of the galactic H I supershells
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6423214
The majority of the shell and supershell formations typical of the galactic distribution of neutral hydrogen probably do not result from the impact of supernova remnants or stellar wind on the interstellar medium, but reflect normal, stratified spiral structure.
- Research Organization:
- Special Astrophysical Observatory, USSR Academy of Sciences, Nizhnii Arkhyz
- OSTI ID:
- 6423214
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 8:2; ISSN SALED
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CONFIGURATION
COSMIC GASES
COSMIC RADIO SOURCES
DISTRIBUTION
FLUIDS
GASES
H1 REGIONS
INTERSTELLAR SPACE
SHELLS
SPACE
SPATIAL DISTRIBUTION
SPIRAL CONFIGURATION
STELLAR WINDS
SUPERNOVA REMNANTS
SYNTHESIS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CONFIGURATION
COSMIC GASES
COSMIC RADIO SOURCES
DISTRIBUTION
FLUIDS
GASES
H1 REGIONS
INTERSTELLAR SPACE
SHELLS
SPACE
SPATIAL DISTRIBUTION
SPIRAL CONFIGURATION
STELLAR WINDS
SUPERNOVA REMNANTS
SYNTHESIS