Historic mass loss from the RS Ophiuchi system

Jacco Th. van Loon (Keele University; UK)

Historic mass loss from the RS Ophiuchi system

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arxiv 0710.5628 v1 pith:KDUDBE5S submitted 2007-10-30 astro-ph

Jacco Th. van Loon (Keele University , UK) This is my paper · ORCID

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keywords dusteruptionsevidencenovaophiuchirecurrentaffectedbeen

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Dust 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.

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Association between Recurrent Novae and Nova Super-Remnants
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A review of nova super-remnants: the prototypical M31N 2008-12a remnant, new Galactic examples around KT Eridani and RS Ophiuchi, and a survey finding none in M31 or the LMC.

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