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

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

Faculty of Computing, Engineering and Science

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

Abstract

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.

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	246
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

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Harman, D. J., Bode, M. F., Darnley, M. J., O’Brien, T. J., Bond, H. E., Starrfield, S., Evans, A., Eyres, S., Ribeiro, V. A. R. M., & Echevarría, J. M. (2008). Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of 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. 246). Astronomical Society of the Pacific.

Harman, D. J. ; Bode, M. F. ; Darnley, M. J. et al. / Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi. RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series. editor / A. Evans ; M. Bode ; T. J. O'Brien ; M. J. Darnley. Vol. 401 Astronomical Society of the Pacific, 2008. pp. 246

@inproceedings{71b777b005f6433faab19185b32a0d78,

title = "Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi",

abstract = "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.",

author = "Harman, {D. J.} and Bode, {M. F.} and Darnley, {M. J.} and O{\textquoteright}Brien, {T. J.} and Bond, {H. E.} and S. Starrfield and A. Evans and Stewart Eyres and Ribeiro, {Val{\'e}rio A. R. M.} and Echevarr{\'i}a, {J. M.}",

year = "2008",

month = dec,

language = "English",

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

volume = "401",

pages = "246",

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",

}

Harman, DJ, Bode, MF, Darnley, MJ, O’Brien, TJ, Bond, HE, Starrfield, S, Evans, A, Eyres, S, Ribeiro, VARM & Echevarría, JM 2008, Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of 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. 246, RS OPHIUCHI (2006) AND THE RECURRENT NOVA PHENOMENON, Keele, United Kingdom, 12/06/07.

Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi. / Harman, D. J.; Bode, M. F.; Darnley, M. 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. 246.

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

TY - GEN

T1 - Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi

AU - Harman, D. J.

AU - Bode, M. F.

AU - Darnley, M. J.

AU - O’Brien, T. J.

AU - Bond, H. E.

AU - Starrfield, S.

AU - Evans, A.

AU - Eyres, Stewart

AU - Ribeiro, Valério A. R. M.

AU - Echevarría, J. M.

PY - 2008/12

Y1 - 2008/12

N2 - 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.

AB - 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.

M3 - Conference contribution

SN - 978-1-58381-674-5

VL - 401

SP - 246

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 -

Harman DJ, Bode MF, Darnley MJ, O’Brien TJ, Bond HE, Starrfield S et al. Hubble Space Telescope Imaging of the Expanding Nebular Remnant of the 2006 Outburst of RS Ophiuchi. In Evans A, Bode M, O'Brien TJ, Darnley MJ, editors, RS Ophiuchi (2006) and the Recurrent Nova Phenomenon: Astronomical Society of the Pacific Conference Series. Vol. 401. Astronomical Society of the Pacific. 2008. p. 246

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

Abstract

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