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Toledo-Roy, J.C.; Velázquez, P.F.; Esquivel, A.; Giacani, E. "A blowout numerical model for the supernova remnant G352.7-0.1" (2013) Monthly Notices of the Royal Astronomical Society. 437(1):898-905
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Abstract:

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. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Published by Oxford University Press on behalf of the Royal Astronomical Society.

Registro:

Documento: Artículo
Título:A blowout numerical model for the supernova remnant G352.7-0.1
Autor:Toledo-Roy, J.C.; Velázquez, P.F.; Esquivel, A.; Giacani, E.
Filiación:Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Ap.P. 70-543 04510 DF, Mexico
Instituto de Astronomía y Física del Espacio (CONICET-UBA), CC 67, Suc. 28, 1428 Buenos Aires, Argentina
FADU, University of Buenos Aires, Buenos Aires, Argentina
Palabras clave:Hydrodynamics; ISM: supernova remnants; Methods: numerical; Radiation mechanisms: non-thermal; Radio continuum: ISM
Año:2013
Volumen:437
Número:1
Página de inicio:898
Página de fin:905
DOI: http://dx.doi.org/10.1093/mnras/stt1955
Título revista:Monthly Notices of the Royal Astronomical Society
Título revista abreviado:Mon. Not. R. Astron. Soc.
ISSN:00358711
CODEN:MNRAA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v437_n1_p898_ToledoRoy

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Citas:

---------- APA ----------
Toledo-Roy, J.C., Velázquez, P.F., Esquivel, A. & Giacani, E. (2013) . A blowout numerical model for the supernova remnant G352.7-0.1. Monthly Notices of the Royal Astronomical Society, 437(1), 898-905.
http://dx.doi.org/10.1093/mnras/stt1955
---------- CHICAGO ----------
Toledo-Roy, J.C., Velázquez, P.F., Esquivel, A., Giacani, E. "A blowout numerical model for the supernova remnant G352.7-0.1" . Monthly Notices of the Royal Astronomical Society 437, no. 1 (2013) : 898-905.
http://dx.doi.org/10.1093/mnras/stt1955
---------- MLA ----------
Toledo-Roy, J.C., Velázquez, P.F., Esquivel, A., Giacani, E. "A blowout numerical model for the supernova remnant G352.7-0.1" . Monthly Notices of the Royal Astronomical Society, vol. 437, no. 1, 2013, pp. 898-905.
http://dx.doi.org/10.1093/mnras/stt1955
---------- VANCOUVER ----------
Toledo-Roy, J.C., Velázquez, P.F., Esquivel, A., Giacani, E. A blowout numerical model for the supernova remnant G352.7-0.1. Mon. Not. R. Astron. Soc. 2013;437(1):898-905.
http://dx.doi.org/10.1093/mnras/stt1955