On the properties of H I shells in the Small Magellanic Cloud

Monthly Notices of the Royal Astronomical Society

Volumn 360, Issue 3, 2005, Pages 1171-1184

  Hatzidimitriou, D ^a   Stanimirovic, S ^b   Maragoudaki, F ^c   Staveley Smith, L ^d   Dapergolas, A ^e   Bratsolis, E ^f  

^a UNIVERSITY OF CRETE   (Greece)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF ATHENS   (Greece)

^d CSIRO   (Australia)

^e NATIONAL OBSERVATORY OF ATHENS   (Greece)

^f TELECOM PARISTECH   (France)

Author keywords

ISM: bubbles; ISM: kinematics and dynamics; Magellanic Clouds

Indexed keywords

DISTRIBUTION FUNCTIONS; GALAXIES; GAMMA RAYS; INTELLIGENT SYSTEMS; MONTE CARLO METHODS; SHELLS (STRUCTURES); SUPERNOVAE;

CEPHEIDS; ISM: BUBBLE; ISM: KINEMATICS AND DYNAMICS; MAGELLANIC CLOUDS; NEUTRAL HYDROGEN; OB ASSOCIATION; PROPERTY; SMALL MAGELLANIC CLOUDS; WOLF-RAYET STARS; YOUNG STELLAR OBJECTS;

LUMINANCE;

EID: 22144445657     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09124.x     Document Type: Article

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