Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/18911
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dc.contributor.authorEvans, A.-
dc.contributor.authorWoodward, C. E.-
dc.contributor.authorHelton, L. A.-
dc.contributor.authorvan Loon, J. T.-
dc.contributor.authorBarry, R. K.-
dc.contributor.authorBode, M. F.-
dc.contributor.authorDavis, R. J.-
dc.contributor.authorDrake, J. J.-
dc.contributor.authorEyres, S. P. S.-
dc.contributor.authorGeballe, T. R.-
dc.contributor.authorGehrz, R. D.-
dc.contributor.authorKerr, T.-
dc.contributor.authorKrautter, J.-
dc.contributor.authorLynch, D. K.-
dc.contributor.authorNess, J-U.-
dc.contributor.authorO'Brien, T. J.-
dc.contributor.authorOsborne, J. P.-
dc.contributor.authorPage, K. L.-
dc.contributor.authorRudy, R. J.-
dc.contributor.authorRussell, R. W.-
dc.contributor.authorSchwarz, G.-
dc.contributor.authorStarrfield, S.-
dc.contributor.authorTyne, V. H.-
dc.date.accessioned2012-10-24T09:06:07Z-
dc.date.available2012-10-24T09:06:07Z-
dc.date.issued2007-12-20-
dc.identifier.citationAstrophysical Journal Letters, 2007, 671 (2), pp. L157-L160-
dc.identifier.issn2041-8205-
dc.identifier.urihttp://hdl.handle.net/2381/18911-
dc.identifier.urihttp://iopscience.iop.org/article/10.1086/524944/meta-
dc.description.abstractWe present further Spitzer Space Telescope observations of the recurrent nova RS Ophiuchi, obtained over the period 208-430 days after the 2006 eruption. The later Spitzer IRS data show that the line emission and free-free continuum emission reported earlier is declining, revealing incontrovertible evidence for the presence of silicate emission features at 9.7 and 18 μm. We conclude that the silicate dust survives the hard radiation impulse and shock blast wave from the eruption. The existence of the extant dust may have significant implications for understanding the propagation of shocks through the red giant wind and likely wind geometry.-
dc.language.isoEnglish-
dc.publisherAmerican Astronomical Society, IOP Publishing-
dc.rightsCreative Commons “Attribution Non-Commercial No Derivatives” licence CC BY-NC-ND, further details of which can be found via the following link: http://creativecommons.org/licenses/by-nc-nd/4.0/ Archived with reference to SHERPA/RoMEO and publisher website.-
dc.sourceWeb of Science-
dc.source.urihttp://webofknowledge.com-
dc.subjectScience & Technology-
dc.subjectPhysical Sciences-
dc.subjectAstronomy & Astrophysics-
dc.subjectbinaries : close-
dc.subjectbinaries : symbiotic-
dc.subjectinfrared : stars-
dc.subjectnovae-
dc.subjectcataclysmic variables-
dc.subjectstars : individual (RS Oph)-
dc.subjectSPITZER-SPACE-TELESCOPE-
dc.subjectINFRARED OBSERVATIONS-
dc.subjectSYMBIOTIC STARS-
dc.subjectSHOCK-WAVE-
dc.subjectOUTBURST-
dc.subjectEMISSION-
dc.subjectEVOLUTION-
dc.subjectSPECTRA-
dc.subjectNOVAE-
dc.subjectPHASE-
dc.titleSilicate dust in the environment of RS Ophiuchi following the 2006 eruption-
dc.typeJournal Article-
dc.identifier.doi10.1086/524944-
dc.description.irispid43692-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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