Chandra Cycle 11 Spatial and Spectral Monitoring of SNR1987A

Physics

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Scientific paper

Regular monitoring of SNR1987A, the only supernova remnant in which we can study the early developmental stages in detail, is critical to testing models of remnant evolution, nonequilibrium ionization processes, and thin plasma spectra. SNR1987A presents a unique opportunity to observe the birth and early evolution of a supernova remnant at high spatial and spectral resolution for the first time. We propose to continue our program of monitoring SNR1987A in Cycle 11 at roughly six month intervals.

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