The 2006 explosion of the recurrent nova RS Ophiuchi

T. J. O'Brien; M. F. Bode; R. W. Porcas; T. W.B. Muxlow; R. J. Beswick; S. T. Garrington; S. P.S. Eyres; J. P. Osborne; K. L. Page; A. P. Beardmore; M. R. Goad; S. Starrfield; J. U. Ness; A. Evans; G. K. Skinner; R. J. Davis

The 2006 explosion of the recurrent nova RS Ophiuchi

T. J. O'Brien, M. F. Bode, R. W. Porcas, T. W.B. Muxlow, R. J. Beswick, S. T. Garrington, S. P.S. Eyres, J. P. Osborne, K. L. Page, A. P. Beardmore, M. R. Goad, S. Starrfield, J. U. Ness, A. Evans, G. K. Skinner, R. J. Davis

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Conference article › peer-review

Abstract

RS Ophiuchi is a recurrent nova comprising a white dwarf accreting material from a companion red giant. After 10-30 years, sufficient material accumulates for a thermonuclear explosion to take place on the white dwarf. The ejected matter slams into the wind of the red giant and sets up shocks which result in copious amounts of radio and X-ray emission. Here, we describe observations of the aftermath of the most recent outburst (discovered 12 Feb 2006) paying particular attention to VLBA/EVN/MERLIN imaging and Swift X-ray spectroscopy.

Original language	English (US)
Article number	052
Journal	Proceedings of Science
Volume	36
State	Published - 2006
Event	8th European VLBI Network Symposium, EVN 2006 - Torun, Poland Duration: Sep 26 2006 → Sep 29 2006

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title = "The 2006 explosion of the recurrent nova RS Ophiuchi",

abstract = "RS Ophiuchi is a recurrent nova comprising a white dwarf accreting material from a companion red giant. After 10-30 years, sufficient material accumulates for a thermonuclear explosion to take place on the white dwarf. The ejected matter slams into the wind of the red giant and sets up shocks which result in copious amounts of radio and X-ray emission. Here, we describe observations of the aftermath of the most recent outburst (discovered 12 Feb 2006) paying particular attention to VLBA/EVN/MERLIN imaging and Swift X-ray spectroscopy.",

author = "O'Brien, {T. J.} and Bode, {M. F.} and Porcas, {R. W.} and Muxlow, {T. W.B.} and Beswick, {R. J.} and Garrington, {S. T.} and Eyres, {S. P.S.} and Osborne, {J. P.} and Page, {K. L.} and Beardmore, {A. P.} and Goad, {M. R.} and S. Starrfield and Ness, {J. U.} and A. Evans and Skinner, {G. K.} and Davis, {R. J.}",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.; 8th European VLBI Network Symposium, EVN 2006 ; Conference date: 26-09-2006 Through 29-09-2006",

year = "2006",

language = "English (US)",

volume = "36",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

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TY - JOUR

T1 - The 2006 explosion of the recurrent nova RS Ophiuchi

AU - O'Brien, T. J.

AU - Bode, M. F.

AU - Porcas, R. W.

AU - Muxlow, T. W.B.

AU - Beswick, R. J.

AU - Garrington, S. T.

AU - Eyres, S. P.S.

AU - Osborne, J. P.

AU - Page, K. L.

AU - Beardmore, A. P.

AU - Goad, M. R.

AU - Starrfield, S.

AU - Ness, J. U.

AU - Evans, A.

AU - Skinner, G. K.

AU - Davis, R. J.

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

PY - 2006

Y1 - 2006

N2 - RS Ophiuchi is a recurrent nova comprising a white dwarf accreting material from a companion red giant. After 10-30 years, sufficient material accumulates for a thermonuclear explosion to take place on the white dwarf. The ejected matter slams into the wind of the red giant and sets up shocks which result in copious amounts of radio and X-ray emission. Here, we describe observations of the aftermath of the most recent outburst (discovered 12 Feb 2006) paying particular attention to VLBA/EVN/MERLIN imaging and Swift X-ray spectroscopy.

AB - RS Ophiuchi is a recurrent nova comprising a white dwarf accreting material from a companion red giant. After 10-30 years, sufficient material accumulates for a thermonuclear explosion to take place on the white dwarf. The ejected matter slams into the wind of the red giant and sets up shocks which result in copious amounts of radio and X-ray emission. Here, we describe observations of the aftermath of the most recent outburst (discovered 12 Feb 2006) paying particular attention to VLBA/EVN/MERLIN imaging and Swift X-ray spectroscopy.

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UR - http://www.scopus.com/inward/citedby.url?scp=85055492574&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85055492574

SN - 1824-8039

VL - 36

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 052

T2 - 8th European VLBI Network Symposium, EVN 2006

Y2 - 26 September 2006 through 29 September 2006

ER -

The 2006 explosion of the recurrent nova RS Ophiuchi

Abstract

ASJC Scopus subject areas

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