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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Detalles Bibliográficos
Autores principales:	Velázquez, P.F., Vigh, C.D., Reynoso, E.M., Gómez, D.O., Schneiter, E.M.
Formato:	JOUR
Materias:	Hydrodynamics ISM: individual (Kepler SNR) Methods: numerical Shock waves Supernova remnants X-rays: ISM
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	todo:paper_0004637X_v649_n2_p779_Velazquez
record_format	dspace
spelling	todo:paper_0004637X_v649_n2_p779_Velazquez2023-10-03T14:02:04Z Simulated X-ray emission for a runaway model of Kepler's supernova remnant 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. JOUR 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)
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	JOUR
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
url	http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
work_keys_str_mv	AT velazquezpf simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant AT vighcd simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant AT reynosoem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant AT gomezdo simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant AT schneiterem simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
_version_	1782030828932431872

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

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