Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi

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dc.creatorHarman, D. J.
dc.creatorBode, M. F.
dc.creatorDarnley, M. J.
dc.creatorO'Brien, T. J.
dc.creatorBond, H. E.
dc.creatorStarrfield, S.
dc.creatorEvans, A.
dc.creatorEyres, S. P. S.
dc.creatorRibeiro, V. A. R. M.
dc.creatorEchevarria, J. M.
dc.date2008-09-26
dc.date2009-04-24
dc.date.accessioned2026-07-07T13:07:35Z
dc.date.available2026-07-07T13:07:35Z
dc.descriptionWe report {\it Hubble Space Telescope} imaging obtained 155 days and 449 days after the 2006 outburst of RS Ophiuchi. Both epochs show evidence of extended emission, consistent with that seen in earlier radio observations, and a maximum expansion rate of $3200\pm300$ km s$^{-1}$ (in the plane of the sky). The extended structure is consistent with the remnant having a bipolar morphology with an inclination similar to that determined for the binary.
dc.description5 pages, 2 figures, published in ASP conference proceedings Volume 401 "RS Ophiuchi (2006) and the recurrent nova phenomenon", page 246-250
dc.identifierhttps://arxiv.org/abs/0809.4592
dc.identifierhttp://arxiv.org/abs/0809.4592
dc.identifier2009ASPC..401..246H
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228136
dc.subjectAstrophysics
dc.titleHubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi
dc.typetext

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