RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst

Stewart Eyres; Mark Rushton; T. J. O’Brien; Bob Beswick; Tom Muxlow; Richard Davis; G. C. Anupama; T. Prabhu; N. C. Kantharia; M. F. Bode; M. P. Gawroński; R. Feiler; A. Evans

RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst

Stewart Eyres, Mark Rushton, T. J. O’Brien, Bob Beswick, Tom Muxlow, Richard Davis, G. C. Anupama, T. Prabhu, N. C. Kantharia, M. F. Bode, M. P. Gawroński, R. Feiler, A. Evans

Faculty of Computing, Engineering and Science

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

Abstract

We report GHz observations beginning 4.5 days after the discovery of RS Ophiuchi undergoing its 2006 recurrent nova outburst. Observations over the first 60 days are included, enabling us to follow spectral development throughout the three phases of the remnant development. We see dramatic
brightening on days 4 to 7 at 6 GHz and an accompanying increase in other bands, particularly 1.46 GHz, consistent with transition from the initial phase to the adiabatic expansion phase. This is complete by day 13 when the brightness at 5 GHz is apparently declining from an early maximum (compared with 1985 observations). The flux recovered to a second peak by approximately day 40, consistent with behaviour observed in 1985. At all times the spectral index is consistent with combined thermal and non-thermal components. The emission requires at least 4±2×10−7M⊙ of ejecta.

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	256
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

Eyres, S., Rushton, M., O’Brien, T. J., Beswick, B., Muxlow, T., Davis, R., Anupama, G. C., Prabhu, T., Kantharia, N. C., Bode, M. F., Gawroński, M. P., Feiler, R., & Evans, A. (2008). RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst. 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. 256). Astronomical Society of the Pacific.

@inproceedings{fedeb43e3b7a4fd8ae5419709d418ac0,

title = "RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst",

abstract = "We report GHz observations beginning 4.5 days after the discovery of RS Ophiuchi undergoing its 2006 recurrent nova outburst. Observations over the first 60 days are included, enabling us to follow spectral development throughout the three phases of the remnant development. We see dramaticbrightening on days 4 to 7 at 6 GHz and an accompanying increase in other bands, particularly 1.46 GHz, consistent with transition from the initial phase to the adiabatic expansion phase. This is complete by day 13 when the brightness at 5 GHz is apparently declining from an early maximum (compared with 1985 observations). The flux recovered to a second peak by approximately day 40, consistent with behaviour observed in 1985. At all times the spectral index is consistent with combined thermal and non-thermal components. The emission requires at least 4±2×10−7M⊙ of ejecta.",

author = "Stewart Eyres and Mark Rushton and O{\textquoteright}Brien, {T. J.} and Bob Beswick and Tom Muxlow and Richard Davis and Anupama, {G. C.} and T. Prabhu and Kantharia, {N. C.} and Bode, {M. F.} and Gawro{\'n}ski, {M. P.} and R. Feiler and A. Evans",

year = "2008",

month = dec,

language = "English",

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

volume = "401",

pages = "256",

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",

}

Eyres, S, Rushton, M, O’Brien, TJ, Beswick, B, Muxlow, T, Davis, R, Anupama, GC, Prabhu, T, Kantharia, NC, Bode, MF, Gawroński, MP, Feiler, R & Evans, A 2008, RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst. 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. 256, RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON, Keele, United Kingdom, 12/06/07.

RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst. / Eyres, Stewart; Rushton, Mark; O’Brien, T. J. 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. 256.

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

TY - GEN

T1 - RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst

AU - Eyres, Stewart

AU - Rushton, Mark

AU - O’Brien, T. J.

AU - Beswick, Bob

AU - Muxlow, Tom

AU - Davis, Richard

AU - Anupama, G. C.

AU - Prabhu, T.

AU - Kantharia, N. C.

AU - Bode, M. F.

AU - Gawroński, M. P.

AU - Feiler, R.

AU - Evans, A.

PY - 2008/12

Y1 - 2008/12

N2 - We report GHz observations beginning 4.5 days after the discovery of RS Ophiuchi undergoing its 2006 recurrent nova outburst. Observations over the first 60 days are included, enabling us to follow spectral development throughout the three phases of the remnant development. We see dramaticbrightening on days 4 to 7 at 6 GHz and an accompanying increase in other bands, particularly 1.46 GHz, consistent with transition from the initial phase to the adiabatic expansion phase. This is complete by day 13 when the brightness at 5 GHz is apparently declining from an early maximum (compared with 1985 observations). The flux recovered to a second peak by approximately day 40, consistent with behaviour observed in 1985. At all times the spectral index is consistent with combined thermal and non-thermal components. The emission requires at least 4±2×10−7M⊙ of ejecta.

AB - We report GHz observations beginning 4.5 days after the discovery of RS Ophiuchi undergoing its 2006 recurrent nova outburst. Observations over the first 60 days are included, enabling us to follow spectral development throughout the three phases of the remnant development. We see dramaticbrightening on days 4 to 7 at 6 GHz and an accompanying increase in other bands, particularly 1.46 GHz, consistent with transition from the initial phase to the adiabatic expansion phase. This is complete by day 13 when the brightness at 5 GHz is apparently declining from an early maximum (compared with 1985 observations). The flux recovered to a second peak by approximately day 40, consistent with behaviour observed in 1985. At all times the spectral index is consistent with combined thermal and non-thermal components. The emission requires at least 4±2×10−7M⊙ of ejecta.

M3 - Conference contribution

SN - 978-1-58381-674-5

VL - 401

SP - 256

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 -

RS Ophiuchi: Radio Lightcurve Development Following the 2006 Outburst

Abstract

Workshop

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