RADIATION PRESSURE FROM MASSIVE STAR CLUSTERS AS A LAUNCHING MECHANISM FOR SUPER-GALACTIC WINDS
- Author
- MURRAY, Norman1 ; MENARD, Brice1 ; THOMPSON, Todd A2 3
[1] Canadian Institute for Theoretical Astrophysics, 60 St. George Street, University of Toronto, Toronto, ON M5S 3H8, Canada
[2] Department of Astronomy, The Ohio State University, 140 W 18th Avenue, Columbus, OH 43210, United States
[3] Center for Cosmology & Astro-Particle Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210, United States - Source
The Astrophysical journal. 2011, Vol 735, Num 1 ; 66.1-66.12 ; 1 ; ref : 3/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- ISM: structure dust extinction galaxies: star clusters: general intergalactic medium quasars: absorption lines
- Keyword (fr)
- Amas galaxies Amas stellaire Disque galactique Déplacement vers le rouge Etoile massive Formation stellaire Galaxies disques Galaxies à flambée Gaz chaud Matière intergalactique Pression rayonnement Quasar Raie absorption Supernova galactique Taux formation Vent galactique
- Keyword (en)
- Galaxy clusters Star clusters Galactic disks Red shift Massive stars Star formation Disk galaxies Starburst galaxies Hot gas Intergalactic matter Radiation pressure Quasars Absorption line Galactic supernova Formation rate Galactic wind
- Keyword (es)
- Galaxias llamarada estelar Gas caliente Raya absorción Supernova galáctica Grado formación Viento galáctico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 24326401
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
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DOI
10.1088/0004-637X/735/1/66 
https://dx.doi.org/10.1088/0004-637X/735/1/66
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