The Symbiotic PHENOMENA:CONTINUATION of Early Acq pt 2

Details The Symbiotic PHENOMENA:CONTINUATION of Early Acq pt 2 The Symbiotic PHENOMENA:CONTINUATION of Early Acq pt 2

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.4162m&link_type=abstract

HST Proposal ID #4162

Physics

Hst Proposal Id #4162

Scientific paper

Symbiotic stars are interacting binaries. The relevant interaction processes include mass expulsion from a common envelope between the two stars, collimated flows, accretion disk formation around the compact hot star, evolution of outbursts, as well as mass outflow leading to jet-like features with particularly intriguing characteristics. However, the nature of these systems and the physical processes that explain their behavior remain unsettled. Spectroscopy with HRS will decisively advance our knowledge of the kinematical and ionization structure of the central HII region that surrounds the binary. It is hoped that this will finally answer the controversial question concerning the nature of the hot object in symbiotics. High spatial resolution radio

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