Mass-loss from Red Giants

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dc.creatorEspey, Brian
dc.creatorCrowley, Cian
dc.date2008-03-07
dc.date2008-03-13
dc.date.accessioned2026-07-07T09:26:20Z
dc.date.available2026-07-07T09:26:20Z
dc.descriptionAlthough much is known about the nature of winds from hot stars and giants and supergiants with spectral types earlier than K, there is still much to be learned regarding the mass-loss process in cool, late-type stars. We will review the current state of research, with particular reference to observations and modelling of mass-loss from giant stars in symbiotic systems.
dc.descriptionRevised version of review submitted to the RS Oph meeting, Keele 2007
dc.identifierhttps://arxiv.org/abs/0803.1170
dc.identifierhttp://arxiv.org/abs/0803.1170
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/156718
dc.subjectAstrophysics
dc.titleMass-loss from Red Giants
dc.typetext

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