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    Coordinated observations of interacting peculiar red giant binaries, 1 (1995)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: IUE Observations were begun for a two-year program to monitor the UV variability of three interacting peculiar red giant (PRG) binaries, HD 59643 (C6,s) HD 35155 (S3/2), and HR 1105 (S3.5/2.5). All of these systems were suspected to involve accretion of material from the PRG to a white-dwarf secondary, based mainly on previous IUE investigations. From our earlier surveys of PRG's, they were primary candidates to test the hypothesis that Tc-poor PRG's are formed as a result of mass transfer from a secondary component rather than from internal thermal pulsing while on the asymptotic red giant branch.
    Keywords: ASTRONOMY
    Type: NASA-CR-199875 , NAS 1.26:199875 , NIPS-96-08163
    Format: application/pdf
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