Swift Observations of Shock Evolution in RS Ophiuchi

M. F. Bode; J. P. Osborne; K. L. Page; A. P. Beardmore; T. J. O’Brien; J.-U. Ness; S. Starrfield; G. K. Skinner; M. J. Darnley; J. J. Drake; A. Evans; Stewart Eyres; J. Krautter; G. Schwarz

Swift Observations of Shock Evolution in RS Ophiuchi

M. F. Bode, J. P. Osborne, K. L. Page, A. P. Beardmore, T. J. O’Brien, J.-U. Ness, S. Starrfield, G. K. Skinner, M. J. Darnley, J. J. Drake, A. Evans, Stewart Eyres, J. Krautter, G. Schwarz

Cyfadran Cyfrifiadureg, Peirianneg a Gwyddoniaeth

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Our Swift observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with the circumstellar environment. Over the first month, the XRT data are dominated by emission from rapidly evolving shocks. We discuss the differences in derived parameters from those found for RXTE at early times and the evolution of the X-ray emission to much later times. It is apparent that at late times several emission components are present. We find no strong evidence of the proposed shock break-out in our data.

Iaith wreiddiol	Saesneg
Teitl	RS Ophiuchi (2006) and the Recurrent Nova Phenomenon
Is-deitl	Astronomical Society of the Pacific Conference Series
Golygyddion	A. Evans, M. Bode, T. J. O'Brien, M. J. Darnley
Cyhoeddwr	Astronomical Society of the Pacific
Tudalennau	269-269
Cyfrol	401
ISBN (Electronig)	978-1-58381-675-2
ISBN (Argraffiad)	978-1-58381-674-5
Statws	Cyhoeddwyd - Rhag 2008
Digwyddiad	RS 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 2007 → 14 Meh 2007

Gweithdy

Gweithdy	RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON
Gwlad/Tiriogaeth	Y Deyrnas Unedig
Dinas	Keele
Cyfnod	12/06/07 → 14/06/07

Dyfynnu hyn

Bode, M. F., Osborne, J. P., Page, K. L., Beardmore, A. P., O’Brien, T. J., Ness, J.-U., Starrfield, S., Skinner, G. K., Darnley, M. J., Drake, J. J., Evans, A., Eyres, S., Krautter, J., & Schwarz, G. (2008). Swift Observations of Shock Evolution in RS Ophiuchi. Yn A. Evans, M. Bode, T. J. O'Brien, & M. J. Darnley (Gol.), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series (Cyfrol 401, tt. 269-269). Astronomical Society of the Pacific.

@inproceedings{7e8a193d07434abba1429ae0f276c5f2,

title = "Swift Observations of Shock Evolution in RS Ophiuchi",

abstract = "Our Swift observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with the circumstellar environment. Over the first month, the XRT data are dominated by emission from rapidly evolving shocks. We discuss the differences in derived parameters from those found for RXTE at early times and the evolution of the X-ray emission to much later times. It is apparent that at late times several emission components are present. We find no strong evidence of the proposed shock break-out in our data.",

author = "Bode, {M. F.} and Osborne, {J. P.} and Page, {K. L.} and Beardmore, {A. P.} and O{\textquoteright}Brien, {T. J.} and J.-U. Ness and S. Starrfield and Skinner, {G. K.} and Darnley, {M. J.} and Drake, {J. J.} and A. Evans and Stewart Eyres and J. Krautter and G. Schwarz",

year = "2008",

month = dec,

language = "English",

isbn = "978-1-58381-674-5",

volume = "401",

pages = "269--269",

editor = "A. Evans and M. Bode and O'Brien, {T. J.} and Darnley, {M. J. }",

booktitle = "RS Ophiuchi (2006) and the Recurrent Nova Phenomenon",

publisher = "Astronomical Society of the Pacific",

note = "RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON : Proceedings of a workshop held at Keele University, 12-14 June 2007 ; Conference date: 12-06-2007 Through 14-06-2007",

}

Bode, MF, Osborne, JP, Page, KL, Beardmore, AP, O’Brien, TJ, Ness, J-U, Starrfield, S, Skinner, GK, Darnley, MJ, Drake, JJ, Evans, A, Eyres, S, Krautter, J & Schwarz, G 2008, Swift Observations of Shock Evolution in RS Ophiuchi. yn A Evans, M Bode, TJ O'Brien & MJ Darnley (gol.), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series. cyfrol. 401, Astronomical Society of the Pacific, tt. 269-269, RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON, Keele, Y Deyrnas Unedig, 12/06/07.

Swift Observations of Shock Evolution in RS Ophiuchi. / Bode, M. F.; Osborne, J. P.; Page, K. L. et al.
RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series. gol. / A. Evans; M. Bode; T. J. O'Brien; M. J. Darnley. Cyfrol 401 Astronomical Society of the Pacific, 2008. t. 269-269.

Allbwn ymchwil: Pennod mewn Llyfr/Adroddiad/Trafodion Cynhadledd › Cyfraniad i gynhadledd › adolygiad gan gymheiriaid

TY - GEN

T1 - Swift Observations of Shock Evolution in RS Ophiuchi

AU - Bode, M. F.

AU - Osborne, J. P.

AU - Page, K. L.

AU - Beardmore, A. P.

AU - O’Brien, T. J.

AU - Ness, J.-U.

AU - Starrfield, S.

AU - Skinner, G. K.

AU - Darnley, M. J.

AU - Drake, J. J.

AU - Evans, A.

AU - Eyres, Stewart

AU - Krautter, J.

AU - Schwarz, G.

PY - 2008/12

Y1 - 2008/12

N2 - Our Swift observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with the circumstellar environment. Over the first month, the XRT data are dominated by emission from rapidly evolving shocks. We discuss the differences in derived parameters from those found for RXTE at early times and the evolution of the X-ray emission to much later times. It is apparent that at late times several emission components are present. We find no strong evidence of the proposed shock break-out in our data.

AB - Our Swift observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with the circumstellar environment. Over the first month, the XRT data are dominated by emission from rapidly evolving shocks. We discuss the differences in derived parameters from those found for RXTE at early times and the evolution of the X-ray emission to much later times. It is apparent that at late times several emission components are present. We find no strong evidence of the proposed shock break-out in our data.

M3 - Conference contribution

SN - 978-1-58381-674-5

VL - 401

SP - 269

EP - 269

BT - RS Ophiuchi (2006) and the Recurrent Nova Phenomenon

A2 - Evans, A.

A2 - Bode, M.

A2 - O'Brien, T. J.

A2 - Darnley, M. J.

PB - Astronomical Society of the Pacific

T2 - RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON

Y2 - 12 June 2007 through 14 June 2007

ER -

Swift Observations of Shock Evolution in RS Ophiuchi

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