X-Ray Observations of SN 1006 with Integral

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dc.creatorKalemci, E.
dc.creatorReynolds, S. P.
dc.creatorBoggs, S. E.
dc.creatorLund, N.
dc.creatorChenevez, J.
dc.creatorRenaud, M.
dc.creatorRho, J.
dc.date2006-02-15
dc.date.accessioned2026-07-07T13:09:05Z
dc.date.available2026-07-07T13:09:05Z
dc.descriptionThe remnant of the supernova of 1006 AD, the remnant first showing evidence for the presence of X-ray synchrotron emission from shock-accelerated electrons, was observed for ~1000 ksec with INTEGRAL for the study of electron acceleration to very high energies. The aim of the observation was to characterize the synchrotron emission, and attempt to detect non-thermal bremsstrahlung, using the combination of IBIS and JEM-X spatial and spectral coverage. The source was detected with JEM-X between 2.4 and 8.4 keV bands, and not detected with either ISGRI or SPI above 20 keV. The ISGRI upper limit is about a factor of four above current model predictions, but confirms the presence of steepening in the power-law extrapolated from lower energies (< 4 keV).
dc.description5 pages, 3 figures, 1 table, accepted for publication in the Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0602335
dc.identifierhttp://arxiv.org/abs/astro-ph/0602335
dc.identifierAstrophys.J.644:274-278,2006
dc.identifierdoi:10.1086/503377
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228619
dc.subjectAstrophysics
dc.titleX-Ray Observations of SN 1006 with Integral
dc.typetext

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