Atmospheric Structure of Hybrid Giants

Details Atmospheric Structure of Hybrid Giants Atmospheric Structure of Hybrid Giants

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8035l&link_type=abstract

HST Proposal ID #8035

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Hst Proposal Id #8035 Cool Stars

Scientific paper

Modes E140M, E230M, and E230H will be used to construct a complete UV spectral atlas of Alpha TrA, which is one of the brightest hybrid-chromosphere stars. The atlas will be used to study both the wind and the high temperature lines. Line fluxes will be used to construct a detailed emission measure model and to determine the electron density. The line profiles will be studied for evidence o f bulk motions, turbulent motions, and heating mechanisms. Analysis of the Mg II, Fe II, and other lines will provide information on the wind acceleration.

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