On the properties of H I shells in the small magellanic cloud

Author

HATZIDIMITRIOU, D¹ ; STANIMIROVIC, S² ; MARAGOUDAKI, F³ ; STAVELEY-SMITH, L⁴ ; DAPERGOLAS, A⁵ ; BRATSOLIS, E⁶
[1] Physics Department, University of Crete, PO Box 2208, 710-03 Heraklion, Crete, Greece
[2] Radio Astronomy Laboratory, University of California, Berkeley, 601 Campbell Hall, Berkeley, CA 94720, United States
[3] Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Athens, 15784 Athens, Greece
[4] Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia
[5] Astronomical Institute, National Observatory of Athens, PO Box 20048, 11810 Athens, Greece
[6] Department Traitement du Signal et des Images, Ecole Nationale Superieure des Telecommunications, Telecom Paris, 46 rue Barrault, 75634, France

Source

Monthly Notices of the Royal Astronomical Society. 2005, Vol 360, Num 3, pp 1171-1184, 14 p ; ref : 64 ref

CODEN

MNRAA4

ISSN

0035-8711

Scientific domain

Astronomy earth cosmic environment

Publisher

Blackwell Science, Oxford

Publication country

United Kingdom

Document type

Article

Language

English

Author keyword

ISM: bubbles ISM: kinematics and dynamics Magellanic Clouds

Keyword (fr)

Age Amas stellaire Association stellaire OB Catalogue astronomique Cinématique Céphéide Dynamique Etoile type Wolf Rayet Explosion supernova Fonction distribution vitesse Formation stellaire Hydrogène neutre Loi puissance Luminosité Modèle standard Mécanisme formation Méthode Monte Carlo Nuages Magellan Objet stellaire jeune Petit Nuage Magellan Reste supernova Supergéante Sursaut Rγ Turbulence Vent stellaire Vitesse expansion

Keyword (en)

Age Star clusters OB stellar association Astronomical catalogues Kinematics Cepheids Dynamics Wolf-Rayet stars Supernovae explosion Velocity distribution function Star formation Neutral hydrogen Power law Luminosity Standard model Formation mechanism Monte Carlo methods Magellanic Clouds Young stellar object Small Magellanic Cloud Supernova remnants Supergiant stars Gamma ray burst Turbulence Stellar winds Expansion velocity

Keyword (es)

Edad Asociación estelar OB Explosión supernova Función distribución velocidad Hidrógeno neutro Ley poder Mecanismo formacion Objeto estelar joven Arrebato Rγ Velocidad expansión

Discipline

Astronomy

Origin

Inist-CNRS

Database

PASCAL

INIST identifier

16876441

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS