Mm/submm observations of symbiotic binary stars

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dc.creatorMikolajewska, J.
dc.creatorIvison, R. J.
dc.creatorOmont, A.
dc.date2002-10-22
dc.date.accessioned2026-07-07T02:05:48Z
dc.date.available2026-07-07T02:05:48Z
dc.descriptionWe present and discuss mm/submm observations of quiescent S-type symbiotic systems, and compare them with popular models proposed to account for their radio emission. We find that the M giant mass-loss rates derived from our observations are systematically higher than those reported for single M giants.
dc.description4 pages, 2 figures. To appear in 'Symbiotic stars probing stellar evolution', eds. R.M.L. Corradi, J. Mikolajewska, T. Mahoney
dc.identifierhttps://arxiv.org/abs/astro-ph/0210491
dc.identifierhttp://arxiv.org/abs/astro-ph/0210491
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5215
dc.subjectAstrophysics
dc.titleMm/submm observations of symbiotic binary stars
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