Numerical model for the SNR DEM L316: Simulated X-ray emission
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. Synthet...
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todo:paper_00358711_v395_n1_p351_ToledoRoy2023-10-03T14:46:53Z Numerical model for the SNR DEM L316: Simulated X-ray emission Toledo-Roy, J.C. Velázquez, P.F. De Colle, F. González, R.F. Reynoso, E.M. Kurtz, S.E. Reyes-Iturbide, J. Conduction Hydrodynamics Magellanic Clouds Methods: numerical Supernova remnants X-rays: individual: DEM L316 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. Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Reynoso, E.M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v395_n1_p351_ToledoRoy |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Conduction Hydrodynamics Magellanic Clouds Methods: numerical Supernova remnants X-rays: individual: DEM L316 |
| spellingShingle |
Conduction Hydrodynamics Magellanic Clouds Methods: numerical Supernova remnants X-rays: individual: DEM L316 Toledo-Roy, J.C. Velázquez, P.F. De Colle, F. González, R.F. Reynoso, E.M. Kurtz, S.E. Reyes-Iturbide, J. Numerical model for the SNR DEM L316: Simulated X-ray emission |
| topic_facet |
Conduction Hydrodynamics Magellanic Clouds Methods: numerical Supernova remnants X-rays: individual: DEM L316 |
| description |
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. |
| format |
JOUR |
| author |
Toledo-Roy, J.C. Velázquez, P.F. De Colle, F. González, R.F. Reynoso, E.M. Kurtz, S.E. Reyes-Iturbide, J. |
| author_facet |
Toledo-Roy, J.C. Velázquez, P.F. De Colle, F. González, R.F. Reynoso, E.M. Kurtz, S.E. Reyes-Iturbide, J. |
| author_sort |
Toledo-Roy, J.C. |
| title |
Numerical model for the SNR DEM L316: Simulated X-ray emission |
| title_short |
Numerical model for the SNR DEM L316: Simulated X-ray emission |
| title_full |
Numerical model for the SNR DEM L316: Simulated X-ray emission |
| title_fullStr |
Numerical model for the SNR DEM L316: Simulated X-ray emission |
| title_full_unstemmed |
Numerical model for the SNR DEM L316: Simulated X-ray emission |
| title_sort |
numerical model for the snr dem l316: simulated x-ray emission |
| url |
http://hdl.handle.net/20.500.12110/paper_00358711_v395_n1_p351_ToledoRoy |
| work_keys_str_mv |
AT toledoroyjc numericalmodelforthesnrdeml316simulatedxrayemission AT velazquezpf numericalmodelforthesnrdeml316simulatedxrayemission AT decollef numericalmodelforthesnrdeml316simulatedxrayemission AT gonzalezrf numericalmodelforthesnrdeml316simulatedxrayemission AT reynosoem numericalmodelforthesnrdeml316simulatedxrayemission AT kurtzse numericalmodelforthesnrdeml316simulatedxrayemission AT reyesiturbidej numericalmodelforthesnrdeml316simulatedxrayemission |
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1807316684389744640 |