Geometry of the acceleration in the bipolar supernova remnant of SN 1006

Details Geometry of the acceleration in the bipolar supernova remnant of SN 1006 Geometry of the acceleration in the bipolar supernova remnant of SN 1006

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..138d&link_type=abstract

XMM-Newton Proposal ID #06538601

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Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Sn 1006-Sw

Scientific paper

We propose a detailed study of the acceleration of particles in the south-west rim of SN 1006 to determine the geometry of the acceleration in this prototype of the class of radio bipolar supernova remnants. To reach our goal, we need to characterize the following quantities in both synchrotron rims all along the shock at the scale of the width of the synchrotron filaments: cut-off frequency of the synchrotron spectrum and downstream magnetic field, together with estimates of the level of spectral and hydrodynamical back-reaction. Our previous LP on SN 1006 provides these quantities for the north-east rim, but not for the south-west rim which hence has insufficient statistics. To achieve the above objectives, we need a new observation of 120 ks of the south-west rim.

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