XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source

The observations of the supernova remnant (SNR) RX J1713.7-3946 performed in five distinct pointings with the EPIC instrument on board the satellite XMM-Newton were presented. RX J1713.7-3946 is a shell type SNR dominated by synchrotron radiation in the X-rays. Its emission and absorption along the...

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Autores principales: Cassam-Chenaï, G., Decourchelle, A., Ballet, J., Sauvageot, J.-L., Dubner, G., Giacani, E.
Formato: JOUR
Materias:
Acceleration of particles
ISM: supernova remnants ISM: individual objects: G347.3-0.5 (RXJ1713.7-3946)
Radiation mechanisms: non-thermal
X-rays: ISM-stars: individual: 1WGA j1713.4-3949
Absorption
Diffusion
Electrons
Galaxies
Photons
Shock waves
Spectrum analysis
Synchrotron radiation
X rays
Molecular clouds
Photon index
Supernova remnant (SNR)
X-ray emission
Astrophysics
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v427_n1_p199_CassamChenai
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id todo:paper_00046361_v427_n1_p199_CassamChenai
record_format dspace
spelling todo:paper_00046361_v427_n1_p199_CassamChenai2023-10-03T14:00:09Z XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source Cassam-Chenaï, G. Decourchelle, A. Ballet, J. Sauvageot, J.-L. Dubner, G. Giacani, E. Acceleration of particles ISM: supernova remnants ISM: individual objects: G347.3-0.5 (RXJ1713.7-3946) Radiation mechanisms: non-thermal X-rays: ISM-stars: individual: 1WGA j1713.4-3949 Absorption Diffusion Electrons Galaxies Photons Shock waves Spectrum analysis Synchrotron radiation X rays Molecular clouds Photon index Supernova remnant (SNR) X-ray emission Astrophysics The observations of the supernova remnant (SNR) RX J1713.7-3946 performed in five distinct pointings with the EPIC instrument on board the satellite XMM-Newton were presented. RX J1713.7-3946 is a shell type SNR dominated by synchrotron radiation in the X-rays. Its emission and absorption along the line-of-sight was characterized over the entire SNR. The X-ray mapping of the absorbing column density revealed strong well-constrained variations and a strong absorption in the southwest. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v427_n1_p199_CassamChenai
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Acceleration of particles
ISM: supernova remnants ISM: individual objects: G347.3-0.5 (RXJ1713.7-3946)
Radiation mechanisms: non-thermal
X-rays: ISM-stars: individual: 1WGA j1713.4-3949
Absorption
Diffusion
Electrons
Galaxies
Photons
Shock waves
Spectrum analysis
Synchrotron radiation
X rays
Molecular clouds
Photon index
Supernova remnant (SNR)
X-ray emission
Astrophysics
spellingShingle Acceleration of particles
ISM: supernova remnants ISM: individual objects: G347.3-0.5 (RXJ1713.7-3946)
Radiation mechanisms: non-thermal
X-rays: ISM-stars: individual: 1WGA j1713.4-3949
Absorption
Diffusion
Electrons
Galaxies
Photons
Shock waves
Spectrum analysis
Synchrotron radiation
X rays
Molecular clouds
Photon index
Supernova remnant (SNR)
X-ray emission
Astrophysics
Cassam-Chenaï, G.
Decourchelle, A.
Ballet, J.
Sauvageot, J.-L.
Dubner, G.
Giacani, E.
XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
topic_facet Acceleration of particles
ISM: supernova remnants ISM: individual objects: G347.3-0.5 (RXJ1713.7-3946)
Radiation mechanisms: non-thermal
X-rays: ISM-stars: individual: 1WGA j1713.4-3949
Absorption
Diffusion
Electrons
Galaxies
Photons
Shock waves
Spectrum analysis
Synchrotron radiation
X rays
Molecular clouds
Photon index
Supernova remnant (SNR)
X-ray emission
Astrophysics
description The observations of the supernova remnant (SNR) RX J1713.7-3946 performed in five distinct pointings with the EPIC instrument on board the satellite XMM-Newton were presented. RX J1713.7-3946 is a shell type SNR dominated by synchrotron radiation in the X-rays. Its emission and absorption along the line-of-sight was characterized over the entire SNR. The X-ray mapping of the absorbing column density revealed strong well-constrained variations and a strong absorption in the southwest.
format JOUR
author Cassam-Chenaï, G.
Decourchelle, A.
Ballet, J.
Sauvageot, J.-L.
Dubner, G.
Giacani, E.
author_facet Cassam-Chenaï, G.
Decourchelle, A.
Ballet, J.
Sauvageot, J.-L.
Dubner, G.
Giacani, E.
author_sort Cassam-Chenaï, G.
title XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
title_short XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
title_full XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
title_fullStr XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
title_full_unstemmed XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
title_sort xmm-newton observations of the supernova remnant rx j1713.7-3946 and its central source
url http://hdl.handle.net/20.500.12110/paper_00046361_v427_n1_p199_CassamChenai
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