IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
A blowout numerical model for the supernova remnant G352.7-0.1
Autor/es:
TOLEDO ROY, J.,C.; VELAZQUEZ, P.; ESQUIVEL, A.; GIACANI, E.
Revista:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Editorial:
WILEY-BLACKWELL PUBLISHING, INC
Referencias:
Lugar: Londres; Año: 2014 p. 898 - 905
ISSN:
0035-8711
Resumen:
We present 3D hydrodynamical simulations of the Galactic supernova
remnant G352.7-0.1. This remnant is peculiar for having a shell-like
inner ring structure and an outer arc in radio observations. In our
model, the supernova explosion producing the remnant occurs inside and
near the border of a spherical cloud with a density higher than that of
the surrounding interstellar medium. A blowout is produced when the
remnant reaches the border of the cloud. We have then used the results
of our hydrodynamical simulations to calculate synthetic synchrotron
radio emission maps, as well as synthetic X-ray maps. For some
combinations of the particle acceleration mechanism and the direction of
the line of sight, our radio maps display the peculiar morphology of
G352.7-0.1 and reproduce the correct relative sizes of the main observed
features. At the same time, the calculated X-ray maps reproduce the
centrally peaked morphology of the observations.