On the origin of the jet-like radio/X-ray morphology of G290.1-0.8

<b>Context.</b> The origin and evolution of supernova remnants of the mixed-morphology class is not well understood. Several remnants present distorted radio or X-ray shells with jet-like structures. G290.1-0.8 (MSH 11-61A) belongs to this particular class. <b>Aims.</b> We a...

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Detalles Bibliográficos
Autores principales:	García, Federico, Combi, Jorge Ariel, Albacete Colombo, Juan Facundo, Romero, Gustavo Esteban, Bocchino, F., López Santiago, J.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas Rayos X ISM: individual objects: G290.1 ISM: supernova remnants Radiation mechanisms: thermal X-rays: ISM G290.1–0.8
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84599
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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