Comprehensive STIS Spectroscopy of the Supernova Remnant 1987A's Formation

Details Comprehensive STIS Spectroscopy of the Supernova Remnant 1987A's Formation Comprehensive STIS Spectroscopy of the Supernova Remnant 1987A's Formation

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.9328c&link_type=abstract

HST Proposal ID #9328

Computer Science

Hst Proposal Id #9328

Scientific paper

The visible consequences of the hard shock of the impact of SN 1987A's ejecta upon the inner circumstellar ring are apparent and developing rapidly. Over the past year, this phenomenon has made a transition, from emission originating in just a few "hot spots" at restricted locations in position angle {PA} around the ER, to a collision producing optical emission over a nearly continuous distribution {with few breaks larger than 45 degrees in PA} and indications of low-level emission arising from nearly all PAs. We propose a modest but effective program to trace superbly the development of the entire interaction region by drawing on capabilities of STIS which are well-matched to the task, and on the strength of comparison with existing STIS data.

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