An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302

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dc.contributor.authorJ. A. Combi
dc.contributor.authorJ. F. Albacete-Colombo
dc.contributor.authorJ. López‐Santiago
dc.contributor.authorGustavo E. Romero
dc.contributor.authorE. Sánchez-Ayaso
dc.contributor.authorJ. Martı́
dc.contributor.authorPedro L. Luque‐Escamilla
dc.contributor.authorPablo G. Pérez‐González
dc.contributor.authorA. J. Muñoz‐Arjonilla
dc.contributor.authorJ. R. Sánchez-Sutil
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T14:46:59Z
dc.date.available2026-03-22T14:46:59Z
dc.date.issued2010
dc.descriptionCitaciones: 15
dc.description.abstractAims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Methods. The morphology and spectral properties of the remnant and the central X-ray point-like source were studied using data from the XMM-Newton and Chandra satellites. Archival radio data and infrared Spitzer observations at 8 and 24 m were used to compare and study its multi-band properties at different wavelengths.
dc.identifier.doi10.1051/0004-6361/200913735
dc.identifier.urihttps://doi.org/10.1051/0004-6361/200913735
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/48516
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy and Astrophysics
dc.sourceUniversidad Nacional de La Plata
dc.subjectSupernova remnant
dc.subjectX-ray
dc.subjectPhysics
dc.subjectObject (grammar)
dc.subjectPoint (geometry)
dc.subjectPoint source
dc.subjectCenter (category theory)
dc.subjectAstrophysics
dc.subjectSupernova
dc.subjectAstronomy
dc.titleAn X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302
dc.typearticle

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