Imaging Supernova Remnant 1987A at the Highest Resolution

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Scientific paper

HRC observations of SN 1987A have revealed the detailed morphology of the remnant, allowing robust measurements of the size and other geometric parameters. We propose a second epoch HRC observation which will indicate the source evolution. The results will be combined with ACIS and radio data to serve as inputs to our hydrodynamic simulations, with the aim to determine the structure of the underlying circumstellar material. We note that the proposed HRC observation will complement rather than conflict with any ACIS observations of SN 1987A, since ACIS data carry spectral information, while HRC data have superior spatial resolution.

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