Historic mass loss from the RS Ophiuchi system

dc.creatorvan Loon, Jacco Th.
dc.date2007-10-30
dc.date.accessioned2026-07-07T08:39:28Z
dc.date.available2026-07-07T08:39:28Z
dc.descriptionDust has been detected in the recurrent nova RS Ophiuchi on several occassions. I model the historical mid-infrared photometry and a recent Spitzer Space Telescope spectrum taken only half a year after the 2006 eruption. The dust envelope is little affected by the eruptions. I show evidence that the eruptions and possibly the red giant wind of RS Oph may sculpt the interstellar medium, and show similar evidence for the recurrent dwarf nova T Pyxidis.
dc.description10 pages, 10 figures including colour images. To appear in "RS Ophiuchi (2006) and the recurrent nova phenomenon", eds. A. Evans, M.F. Bode & T.J. O'Brien, ASP Conf.Ser
dc.identifierhttps://arxiv.org/abs/0710.5628
dc.identifierhttp://arxiv.org/abs/0710.5628
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141080
dc.subjectAstrophysics
dc.titleHistoric mass loss from the RS Ophiuchi system
dc.typetext

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