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

D. J. Harman, M. F. Bode, M. J. Darnley, T. J. O’Brien, H. E. Bond, S. Starrfield, A. Evans, Stewart Eyres, Valério A. R. M. Ribeiro, J. M. Echevarría

Allbwn ymchwil: Pennod mewn Llyfr/Adroddiad/Trafodion CynhadleddCyfraniad i gynhadleddadolygiad gan gymheiriaid

Crynodeb

We report 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±300 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.
Iaith wreiddiolSaesneg
TeitlRS Ophiuchi (2006) and the Recurrent Nova Phenomenon
Is-deitlAstronomical Society of the Pacific Conference Series
GolygyddionA. Evans, M. Bode, T. J. O'Brien, M. J. Darnley
CyhoeddwrAstronomical Society of the Pacific
Tudalennau246
Cyfrol401
ISBN (Electronig)978-1-58381-675-2
ISBN (Argraffiad)978-1-58381-674-5
StatwsCyhoeddwyd - Rhag 2008
DigwyddiadRS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON: Proceedings of a workshop held at Keele University, 12-14 June 2007 - Keele University, Keele, Y Deyrnas Unedig
Hyd: 12 Meh 200714 Meh 2007

Gweithdy

GweithdyRS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON
Gwlad/TiriogaethY Deyrnas Unedig
DinasKeele
Cyfnod12/06/0714/06/07

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