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.

Guardado en:
Detalles Bibliográficos
Autores principales: Velázquez, Pablo Fabián, Vigh, Carlos Donato, Reynoso, Estela Marta, Gomez, Daniel Osvaldo
Publicado: 2006
Materias:
Hydrodynamics
ISM: individual (Kepler SNR)
Methods: numerical
Shock waves
Supernova remnants
X-rays: ISM
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v649_n2_p779_Velazquez
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 paper:paper_0004637X_v649_n2_p779_Velazquez
record_format dspace
spelling paper:paper_0004637X_v649_n2_p779_Velazquez2023-06-08T14:28:52Z Simulated X-ray emission for a runaway model of Kepler's supernova remnant Velázquez, Pablo Fabián Vigh, Carlos Donato Reynoso, Estela Marta Gomez, Daniel Osvaldo 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 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v649_n2_p779_Velazquez 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, Pablo Fabián
Vigh, Carlos Donato
Reynoso, Estela Marta
Gomez, Daniel Osvaldo
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.
author Velázquez, Pablo Fabián
Vigh, Carlos Donato
Reynoso, Estela Marta
Gomez, Daniel Osvaldo
author_facet Velázquez, Pablo Fabián
Vigh, Carlos Donato
Reynoso, Estela Marta
Gomez, Daniel Osvaldo
author_sort Velázquez, Pablo Fabián
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 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v649_n2_p779_Velazquez
http://hdl.handle.net/20.500.12110/paper_0004637X_v649_n2_p779_Velazquez
work_keys_str_mv AT velazquezpablofabian simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT vighcarlosdonato simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT reynosoestelamarta simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
AT gomezdanielosvaldo simulatedxrayemissionforarunawaymodelofkeplerssupernovaremnant
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