Simulated X-ray emission for a runaway model of Kepler's supernova remnant

Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.

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Autores principales: Velázquez, P.F., Vigh, C.D., Reynoso, E.M., Gómez, D.O., Schneiter, E.M.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2006
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
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id paperaa:paper_0004637X_v649_n2_p779_Velazquez
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spelling paperaa:paper_0004637X_v649_n2_p779_Velazquez2023-06-12T16:41:02Z Simulated X-ray emission for a runaway model of Kepler's supernova remnant Astrophys. J. 2006;649(2):779-787 Velázquez, P.F. Vigh, C.D. Reynoso, E.M. Gómez, D.O. Schneiter, E.M. Hydrodynamics ISM: individual (Kepler SNR) Methods: numerical Shock waves Supernova remnants X-rays: ISM Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Vigh, C.D. 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. Fil:Gómez, D.O. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2006 info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion application/pdf eng info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
language Inglés
orig_language_str_mv eng
topic Hydrodynamics
ISM: individual (Kepler SNR)
Methods: numerical
Shock waves
Supernova remnants
X-rays: ISM
spellingShingle Hydrodynamics
ISM: individual (Kepler SNR)
Methods: numerical
Shock waves
Supernova remnants
X-rays: ISM
Velázquez, P.F.
Vigh, C.D.
Reynoso, E.M.
Gómez, D.O.
Schneiter, E.M.
Simulated X-ray emission for a runaway model of Kepler's supernova remnant
topic_facet Hydrodynamics
ISM: individual (Kepler SNR)
Methods: numerical
Shock waves
Supernova remnants
X-rays: ISM
description Fil:Velázquez, P.F. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
format Artículo
Artículo
publishedVersion
author Velázquez, P.F.
Vigh, C.D.
Reynoso, E.M.
Gómez, D.O.
Schneiter, E.M.
author_facet Velázquez, P.F.
Vigh, C.D.
Reynoso, E.M.
Gómez, D.O.
Schneiter, E.M.
author_sort Velázquez, P.F.
title Simulated X-ray emission for a runaway model of Kepler's supernova remnant
title_short Simulated X-ray emission for a runaway model of Kepler's supernova remnant
title_full Simulated X-ray emission for a runaway model of Kepler's supernova remnant
title_fullStr Simulated X-ray emission for a runaway model of Kepler's supernova remnant
title_full_unstemmed Simulated X-ray emission for a runaway model of Kepler's supernova remnant
title_sort simulated x-ray emission for a runaway model of kepler's supernova remnant
publishDate 2006
url http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
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AT reynosoem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT gomezdo simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT schneiterem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
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