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

Faculty of Computing, Engineering and Science

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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.

Original language	English
Title of host publication	RS Ophiuchi (2006) and the Recurrent Nova Phenomenon
Subtitle of host publication	Astronomical Society of the Pacific Conference Series
Editors	A. Evans, M. Bode, T. J. O'Brien, M. J. Darnley
Publisher	Astronomical Society of the Pacific
Pages	269-269
Volume	401
ISBN (Electronic)	978-1-58381-675-2
ISBN (Print)	978-1-58381-674-5
Publication status	Published - Dec 2008
Event	RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON: Proceedings of a workshop held at Keele University, 12-14 June 2007 - Keele University, Keele, United Kingdom Duration: 12 Jun 2007 → 14 Jun 2007

Workshop

Workshop	RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON
Country/Territory	United Kingdom
City	Keele
Period	12/06/07 → 14/06/07

Cite this

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. In A. Evans, M. Bode, T. J. O'Brien, & M. J. Darnley (Eds.), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series (Vol. 401, pp. 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. in A Evans, M Bode, TJ O'Brien & MJ Darnley (eds), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series. vol. 401, Astronomical Society of the Pacific, pp. 269-269, RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON, Keele, United Kingdom, 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. ed. / A. Evans; M. Bode; T. J. O'Brien; M. J. Darnley. Vol. 401 Astronomical Society of the Pacific, 2008. p. 269-269.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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

Abstract

Workshop

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