A multiwavelength study of the supernova remnant G296.8-0.3

We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with complementary radio and infrared data. The spatial and spectral properties of the X-ray emission, detected towards G296.8-0.3, was investigated in order to explore the possible evolutionary scenarios and th...

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Autores principales: Sánchez Ayaso, E., Combi, Jorge Ariel, Albacete Colombo, J. F., Lopez Santiago, J., Martí, J., Muñoz Arjonilla, A. J.
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2011
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/129613
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id I19-R120-10915-129613
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Física
ISM: individual objects: G296.8-0.3
ISM: supernova remnants
X-ray: ISM
Radiation mechanism: thermal
ISM: individual objects: 2XMMi J115836.1-623516
spellingShingle Astronomía
Física
ISM: individual objects: G296.8-0.3
ISM: supernova remnants
X-ray: ISM
Radiation mechanism: thermal
ISM: individual objects: 2XMMi J115836.1-623516
Sánchez Ayaso, E.
Combi, Jorge Ariel
Albacete Colombo, J. F.
Lopez Santiago, J.
Martí, J.
Muñoz Arjonilla, A. J.
A multiwavelength study of the supernova remnant G296.8-0.3
topic_facet Astronomía
Física
ISM: individual objects: G296.8-0.3
ISM: supernova remnants
X-ray: ISM
Radiation mechanism: thermal
ISM: individual objects: 2XMMi J115836.1-623516
description We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with complementary radio and infrared data. The spatial and spectral properties of the X-ray emission, detected towards G296.8-0.3, was investigated in order to explore the possible evolutionary scenarios and the physical connexion with its unusual morphology detected at radio frequencies. G296.8-0.3 displays diffuse X-ray emission correlated with the peculiar radio morphology detected in the interior of the remnant and with the shell-like radio structure observed to the northwest side of the object. The X-ray emission peaks in the soft/medium energy range (0.5–3.0 keV). The X-ray spectral analysis confirms that the column density is high (N; H∼0.64×1022 cm−2) which supports a distant location (d>9 kpc) for the SNR. Its X-ray spectrum can be well represented by a thermal (PSHOCK) model, with kT∼0.86 keV, an ionization timescale of 6.1×1010 cm−3 s, and low abundance (∼0.12 Z; ⊙). The 24 μm observations show shell-like emission correlated with part of the northwest and southeast boundaries of the SNR. In addition a point-like X-ray source is also detected close to the geometrical center of the radio SNR. The object presents some characteristics of the so-called compact central objects (CCO). Its X-ray spectrum is consistent with those found at other CCOs and the value of N; H is consistent with that of G296.8-0.3, which suggests a physical connexion with the SNR.
format Articulo
Preprint
author Sánchez Ayaso, E.
Combi, Jorge Ariel
Albacete Colombo, J. F.
Lopez Santiago, J.
Martí, J.
Muñoz Arjonilla, A. J.
author_facet Sánchez Ayaso, E.
Combi, Jorge Ariel
Albacete Colombo, J. F.
Lopez Santiago, J.
Martí, J.
Muñoz Arjonilla, A. J.
author_sort Sánchez Ayaso, E.
title A multiwavelength study of the supernova remnant G296.8-0.3
title_short A multiwavelength study of the supernova remnant G296.8-0.3
title_full A multiwavelength study of the supernova remnant G296.8-0.3
title_fullStr A multiwavelength study of the supernova remnant G296.8-0.3
title_full_unstemmed A multiwavelength study of the supernova remnant G296.8-0.3
title_sort multiwavelength study of the supernova remnant g296.8-0.3
publishDate 2011
url http://sedici.unlp.edu.ar/handle/10915/129613
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