2nd Epoch High Resolution Spectra of Cassiopeia A: Plasma Evolution and Doppler Mapping

Physics

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Scientific paper

We propose to study the evolution of physical conditions in the bright X-ray ejecta of Cassiopeia A using a 2nd HETGS observation. Based on ACIS observations and plasma evolution models we expect to observe variations in the H- and He-like emission lines of Si and S. This will form an 8-year baseline to the 1st HETGS observation in 2001. We will also use these new data in conjunction with the 1st data set to map the 3-dimensional structure of the dynamically important X-ray ejecta.

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