Computer Science
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1775b&link_type=abstract
IUE Proposal ID #LGGEB
Computer Science
Scientific paper
We want to look for a correlation between temperatures of white dwarf companions of Ba stars and evolutionary state of the Ba stars. We expect to find generally cooler white dwarfs for cooler (i.e., further evolved) Ba stars. Only for the brightest (i.e., generally closest) Ba stars do we have a chance to see those cool white dwarf companions. Only mild Ba stars can be found bright enough. We therefore want to look for white dwarf companions in bright mild Ba stars of advancing spectral types.
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