Gamma-ray emission from massive star forming regions

Recent radio observations support a picture for star formation where there is accretion of matter onto a central protostar with the ejection of molecular outflows that can affect the surrounding medium. The impact of a supersonic outflow on the ambient gas can produce a strong shock that could accel...

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Detalles Bibliográficos
Autores principales:	Araudo, Anabella Teresa, Romero, Gustavo Esteban, Bosch-Ramon, Valentí, Paredes, J. M.
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2008
Materias:	Astronomía Gamma-ray emission Massive stars: formation Radiation mechanisms: non-thermal
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/127373
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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