Chromospheres in Metal Deficient Giant Stars

Details Chromospheres in Metal Deficient Giant Stars Chromospheres in Metal Deficient Giant Stars

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1793d&link_type=abstract

IUE Proposal ID #CCGAD

Physics

Scientific paper

we propose to measure the chromospheric transition Mg II in four red giant stars in globular clusters to define the radiative energy low and structure of the chromosphere in a population of known ages and specific metallicities. Simultaneous high resolution spectroscopy at H-alpha can reveal signatures of mass flow for correlation with chromospheric emission levels.

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