Abstract:
We present a two-component supernova remnant model for the case of Magellanic remnant DEM L316 obtained from two-dimensional, axisymmetric hydrodynamic simulations. We study different scenarios which consider a possible collision between the shells and also the effects of thermal conduction. Synthetic X-ray maps were obtained from numerical results in order to directly compare with the observed morphology of this object. We find a good agreement is achieved when thermal conduction is included, reproducing both the observed morphology and the total X-ray luminosity very well. Finally, our results suggest that the two components of DEM L316 are not in physical interaction. © 2009 RAS.
Registro:
Documento: |
Artículo
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Título: | Numerical model for the SNR DEM L316: Simulated X-ray emission |
Autor: | Toledo-Roy, J.C.; Velázquez, P.F.; De Colle, F.; González, R.F.; Reynoso, E.M.; Kurtz, S.E.; Reyes-Iturbide, J. |
Filiación: | Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Ap.P. 70-543, 04510 D.F., Mexico Dublin Institute for Advanced Studies (DIAS), 31 Fitzwilliam Place, Dublin 2, Ireland Centro de Radioastronomíay Astrofísica, Universidad Nacional Autónoma de México, Apdo. Postal 3-72 (Xangari), Morelia, Michoacán, Mexico Instituto de Astronomíay Física Del Espacio, C.C. 67, suc 28, C.P. 1428, Buenos Aires, Argentina Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Argentina Instituto de Astronomía, Universidad Nacional Autónoma de México, Ap.P. 70-248, 04510 D.F., Mexico
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Palabras clave: | Conduction; Hydrodynamics; Magellanic Clouds; Methods: numerical; Supernova remnants; X-rays: individual: DEM L316 |
Año: | 2009
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Volumen: | 395
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Número: | 1
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Página de inicio: | 351
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Página de fin: | 357
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DOI: |
http://dx.doi.org/10.1111/j.1365-2966.2009.14517.x |
Título revista: | Monthly Notices of the Royal Astronomical Society
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Título revista abreviado: | Mon. Not. R. Astron. Soc.
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ISSN: | 00358711
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CODEN: | MNRAA
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v395_n1_p351_ToledoRoy |
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Citas:
---------- APA ----------
Toledo-Roy, J.C., Velázquez, P.F., De Colle, F., González, R.F., Reynoso, E.M., Kurtz, S.E. & Reyes-Iturbide, J.
(2009)
. Numerical model for the SNR DEM L316: Simulated X-ray emission. Monthly Notices of the Royal Astronomical Society, 395(1), 351-357.
http://dx.doi.org/10.1111/j.1365-2966.2009.14517.x---------- CHICAGO ----------
Toledo-Roy, J.C., Velázquez, P.F., De Colle, F., González, R.F., Reynoso, E.M., Kurtz, S.E., et al.
"Numerical model for the SNR DEM L316: Simulated X-ray emission"
. Monthly Notices of the Royal Astronomical Society 395, no. 1
(2009) : 351-357.
http://dx.doi.org/10.1111/j.1365-2966.2009.14517.x---------- MLA ----------
Toledo-Roy, J.C., Velázquez, P.F., De Colle, F., González, R.F., Reynoso, E.M., Kurtz, S.E., et al.
"Numerical model for the SNR DEM L316: Simulated X-ray emission"
. Monthly Notices of the Royal Astronomical Society, vol. 395, no. 1, 2009, pp. 351-357.
http://dx.doi.org/10.1111/j.1365-2966.2009.14517.x---------- VANCOUVER ----------
Toledo-Roy, J.C., Velázquez, P.F., De Colle, F., González, R.F., Reynoso, E.M., Kurtz, S.E., et al. Numerical model for the SNR DEM L316: Simulated X-ray emission. Mon. Not. R. Astron. Soc. 2009;395(1):351-357.
http://dx.doi.org/10.1111/j.1365-2966.2009.14517.x