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.
@article{arxiv.0710.5628,
title = {Historic mass loss from the RS Ophiuchi system},
author = {Jacco Th. van Loon},
journal= {arXiv preprint arXiv:0710.5628},
year = {2007}
}
Comments
10 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