Physics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..604l&link_type=abstract
Chandra Proposal ID #02500407
Physics
Chandra Proposal Id #02500407
Scientific paper
With fine Balmer filaments marking the location of a shock shown by optical and UV spectroscopy to be moving at 2300 km/s, the NW limb of SN1006 provides a unique environment for understanding physical processes in high-velocity shocks. We propose a 100 ks ACIS-S study of the NW limb to measure the developing ionization and temperature structure 2-20" behind this shock and to characterize the reverse-shocked ejecta. Coupling this Cycle 2 observation of the thermally-dominated NW limb and our Cycle 1 pointing at the synchrotron-dominated NE limb, we will explore the effect of magnetic-field orientation on the development of fast shocks, a crucial step to understanding young SNRs. These studies are possible only with the combination of spatial and spectral resolution available with ACIS.
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