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
Publicado: 2006
Materias:
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v649_n2_p779_Velazquez_oai
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id I28-R145-paper_0004637X_v649_n2_p779_Velazquez_oai
record_format dspace
spelling I28-R145-paper_0004637X_v649_n2_p779_Velazquez_oai2024-08-16 Velázquez, P.F. Vigh, C.D. Reynoso, E.M. Gómez, D.O. Schneiter, E.M. 2006 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. application/pdf http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar Astrophys. J. 2006;649(2):779-787 Hydrodynamics ISM: individual (Kepler SNR) Methods: numerical Shock waves Supernova remnants X-rays: ISM Simulated X-ray emission for a runaway model of Kepler's supernova remnant info:eu-repo/semantics/article info:ar-repo/semantics/artículo info:eu-repo/semantics/publishedVersion https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v649_n2_p779_Velazquez_oai
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-145
collection Repositorio Digital de la Universidad de Buenos Aires (UBA)
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
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_0004637X_v649_n2_p779_Velazquez_oai
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AT reynosoem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT gomezdo simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT schneiterem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
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