G and Early K Giant UV Continua and Early Emission Line Intensities

Details G and Early K Giant UV Continua and Early Emission Line Intensities G and Early K Giant UV Continua and Early Emission Line Intensities

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1766b&link_type=abstract

IUE Proposal ID #CSGEB

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Scientific paper

The continuum flux around 1950A for cool giants is different for otherwise apparently similar stars. For the Hyades this flux is correlated with the chromospheric emission line intensities. We want to study this correlation for other giants. We want to study the systematic changes in emission line and continuum flux along the G to K giant sequence in order to understand the abrupt changes in continuum flux, CIV emission and v(r) sin i observed to occur at spectral types G5III.

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