Optical and Near-IR Monitoring of Symbiotic Binary Systems

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dc.creatorMikolajewska, Joanna
dc.date2001-03-29
dc.date.accessioned2026-07-07T01:58:05Z
dc.date.available2026-07-07T01:58:05Z
dc.descriptionSymbiotic stars are long-period interacting binary systems in which an evolved red giant star transfers material to its much hotter compact companion. Such a composition places them among the most variable stars. In addition to periodic variations due to the binary motion they often show irregular changes due to nova-like eruptions of the hot component. In some systems the cool giant is a pulsating Mira-type star usually surrounded by a variable dust shell. Here, I present results of optical and IR monitoring of symbiotic systems as well as future prospects for such studies.
dc.descriptionInvited paper presented at IAUC 183; 10 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0103496
dc.identifierhttp://arxiv.org/abs/astro-ph/0103496
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2634
dc.subjectAstrophysics
dc.titleOptical and Near-IR Monitoring of Symbiotic Binary Systems
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