XMM-Newton and Chandra observations of G272.2-3.2. Evidence of stellar ejecta in the central region

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Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant G272.2-3.2 in order to obtain important constraints on its ionization stage, the progenitor supernova explosion, and the age of the remnant. Methods. We repo...

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Detalles Bibliográficos
Autores principales: Sánchez Ayaso, E., Combi, Jorge Ariel, Bocchino, F., Albacete Colombo, Juan Facundo, López Santiago, J., Martí, J., Castro, E.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
Materias:
Ciencias Astronómicas
ISM: individual objects: G272.2-3.2
ISM: supernova remnants
Radiation mechanisms: thermal
X-rays: ISM
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85504
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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