Hard X-rays observations of SN 1006 with INTEGRAL

Details Hard X-rays observations of SN 1006 with INTEGRAL Hard X-rays observations of SN 1006 with INTEGRAL

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004head....8.2414k&link_type=abstract

American Astronomical Society, HEAD meeting #8, #24.14; Bulletin of the American Astronomical Society, Vol. 36, p.951

Astronomy and Astrophysics

Astronomy

Scientific paper

The 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 ˜900 ksec with INTEGRAL to study electron acceleration to very high energies. In IBIS and JEM-X spectral bands, both synchrotron emission and bremsstrahlung are expected. The aim of the observations is to distinguish the morphology of synchrotron and bremsstrahlung regions using the combination of IBIS and JEM-X spatial and spectral coverage. Here, we report on our preliminary results from the analysis of the INTEGRAL data.

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