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Outbursts of classical symbiotics: Multi-wavelength observations of the 2000-2001 outburst of Z Andromedae

dc.contributor.authorESPEY, BRIAN RUSSELL
dc.contributor.editorB.T., Gansickeen
dc.contributor.editorK., Beuermannen
dc.contributor.editor&, K. Reinschen
dc.date.accessioned2008-06-19T13:42:35Z
dc.date.available2008-06-19T13:42:35Z
dc.date.issued2002
dc.date.submitted2002en
dc.identifier.citationSokoloski, J.L., Kenyon, S.J., Kong, A.K.H., Charles, P.A., Kaiser, C.R., Seymour, N., Espey, B.R., Keyes, C.D., McCandliss, S.R., Filippenko, A.V., Li, W., Pooley, G.G., Brocksopp, C. and Stone, R.P.S. 'Outbursts of classical symbiotics: Multi-wavelength observations of the 2000-2001 outburst of Z Andromedae' in Astronomical Society of the Pacific Conference Series, The Physics of Cataclysmic Variables and Related Objects, edited by B.T. Gansicke, K. Beuermann, & K. Reinsch , 261, Astronomical Society of the Pacific, 2002, pp. 667 ? 668.en
dc.identifier.issn35471
dc.identifier.otherN
dc.identifier.otherNen
dc.descriptionPUBLISHEDen
dc.description.abstractWe describe the first results from a program of multi-wavelength monitoring of symbiotic binary stars in outburst. The prototypical symbiotic star Z Andromedae was observed extensively at radio, optical, far-UV, and X-ray wavelengths during its current (ongoing) outburst. These observations provide evidence for an initial obscuration or the source of ionizing radiation by an optically thick shell of material, outflow with velocities of 100s of km/s, plus collisional excitation and shock heating of the red-giant wind. In addition, the optical light curve reveals variability on time scales as short as days on both the rise to and decline from optical maximum.en
dc.format.extent667en
dc.format.extent668en
dc.format.extent195519 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseries261en
dc.rightsYen
dc.subjectPhysicsen
dc.titleOutbursts of classical symbiotics: Multi-wavelength observations of the 2000-2001 outburst of Z Andromedaeen
dc.typeConference Paperen
dc.type.supercollectionscholarly_publicationsen
dc.identifier.peoplefinderurlhttp://people.tcd.ie/espeyb
dc.identifier.rssinternalid35471
dc.identifier.rssurihttp://arxiv.org/pdf/astro-ph/0110042v1
dc.identifier.urihttp://hdl.handle.net/2262/17441


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