Highly Evolved Stars of Low Mass - Cycle 1

Details Highly Evolved Stars of Low Mass - Cycle 1 Highly Evolved Stars of Low Mass - Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.4046h&link_type=abstract

HST Proposal ID #4046

Physics

Hst Proposal Id #4046

Scientific paper

I propose to use the HRS to study highly evolved stars, particularly the central stars of planetary nebulae. The study includes (1) an attempt to detect and measure the flux from extremely hot stars (T>150,000 K), (2) an investigation of hydrogen and carbon-rich central stars and their recent ejecta, (3) an investigation of the interaction of the wind from a central star with the surrounding nebula, and (4) follow-up spectroscopic studies of uv-bright stars discovered in globular clusters.

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