VV Cephei Type Stars

Details VV Cephei Type Stars VV Cephei Type Stars

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1898s&link_type=abstract

IUE Proposal ID #VVGJS

Computer Science

Scientific paper

Three new VV Cephei-type stars were discovered by Barbier (1971). We propose to observe these systems to detect and characterize the continuum of the companion and to investigate emission lines from the cool M star and/or by circumstellar material. One star (BD+63 0003) has been monitored extensively by one of the investigators (EFG) and observations would be scheduled about 6 to 9 months apart to coincide with maximum and minimum light in order to detect any dependence of emission activity or interaction with the hot component on the pulsations of the M supergiant component.

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