Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

Context. Efficient particle acceleration can modify the structure of supernova remnants. We present the results of a combined analysis of the XMM-Newton EPIC archive observations of SN 1006.Aims. We attempt to describe the spatial distribution of the physical and chemical properties of the X-ray emi...

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Detalles Bibliográficos
Autores principales: Miceli, M., Bocchino, F., Iakubovskyi, D., Orlando, S., Telezhinsky, I., Kirsch, M.G.F., Petruk, O., Dubner, G., Castelletti, G.
Formato: JOUR
Materias:
ISM: individual objects: SN 1006
ISM: supernova remnants
X-rays: ISM
Aspect angles
Azimuthal variations
Chemical compositions
Combined analysis
Contact discontinuities
Energy band
Interstellar magnetic fields
Line of Sight
MHD models
Nonthermal
Nonthermal emission
Particle acceleration
Physical and chemical properties
Shock fronts
Spatial distribution
Spatially resolved
Spectral analysis
Supernova remnants
Thermal emissions
Thermal images
Thermal x-rays
X ray spectrum
X-ray emitting
X-ray emitting plasmas
XMM-Newton
Chemical properties
Emission spectroscopy
Magnetic fields
Particle accelerator accessories
Size distribution
Spectrum analysis
Spectrum analyzers
Three dimensional
X rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v501_n1_p239_Miceli
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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