Detailed study of SNR G306.3 - 0.9 using XMM-Newton and Chandra observations

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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 (SNR) G306.3-0.9 in detail to obtain constraints on its ionization stage, the progenitor supernova explosion, and the age of the remnant. Methods. We used comb...

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Detalles Bibliográficos
Autores principales: Combi, J.A., García, F., Suárez, A.E., Luque-Escamilla, P.L., Paron, S., Miceli, M.
Formato: JOUR
Materias:
0.9
Infrared: ISM
ISM: individual objects: SNR G306.3
ISM: supernova remnants
Radiation mechanisms: thermal
Radio continuum: ISM
X-rays: ISM
Calcium
Chemical analysis
Electromagnetic wave emission
Geometry
Ionization
Signal to noise ratio
Spectrum analysis
ISM: individual objects
X rays: ISM
Supernovae
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v592_n_p_Combi
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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