IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
artículos
Título:
Evolving Supernova Remnants in Multiphase Interstellar Media
Autor/es:
VILLAGRAN, MARCO A; GIACANI, E B; GÓMEZ, D O; VELÁZQUEZ, P F
Revista:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Editorial:
WILEY-BLACKWELL PUBLISHING, INC
Referencias:
Año: 2019 vol. 491 p. 2855 - 2863
ISSN:
0035-8711
Resumen:
We performed three-dimensional magnetohydrodynamic simulations to study the evolution of asupernova remnant (SNR) in a turbulent neutral atomic interstellar medium. The media used asbackground shares characteristics with the Solar neighbourhood and the SNR has mass and energysimilar to those of a Type Ia object. Our initial conditions consist of dense clouds in a dilutedmedium, with the main difference between simulations being the average magnitude of the magneticfield. We measured amplifications of the magnetic energy of up to 34% and we generated syntheticmaps that illustrate how the same object can show different apparent geometries and physicalproperties when observed through different lines of sight.