Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source

Tim J. O'brien; Stewart P. S. Eyres; Michael F. Bode; J. P. Osborne; K. L. Page; A. P. Beardmore; M.R. Goad; S. Starrfield; J.-u. Ness; J. Krautter; G. Schwarz; D. N.  Burrows; N. Gehrels; J. J.  Drake; A. Evans

doi:10.1088/0004-637X/727/2/124

Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source

Tim J. O'brien, Stewart P. S. Eyres, Michael F. Bode, J. P. Osborne, K. L. Page, A. P. Beardmore, M.R. Goad, S. Starrfield, J.-u. Ness, J. Krautter, G. Schwarz, D. N. Burrows, N. Gehrels, J. J. Drake, A. Evans

Faculty of Computing, Engineering and Science

Research output: Contribution to journal › Article › peer-review

Abstract

V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence. Although V407 Cyg likely hosts a massive accreting white dwarf, making it a candidate progenitor system for a Type Ia supernova, the dense and radially continuous circumbinary material surrounding V407 Cyg is inconsistent with observational constraints on the environments of most Type Ia supernovae.

Original language	English
Journal	The Astrophysical Journal
Volume	727
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/727/2/124
Publication status	Published - 2010

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O'brien, T. J., Eyres, S. P. S., Bode, M. F., Osborne, J. P., Page, K. L., Beardmore, A. P., Goad, M. R., Starrfield, S., Ness, J., Krautter, J., Schwarz, G., Burrows, D. N., Gehrels, N., Drake, J. J., & Evans, A. (2010). Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source. The Astrophysical Journal, 727(2). https://doi.org/10.1088/0004-637X/727/2/124

@article{f76928e2beaf41089faa94a1cd078da1,

title = "Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source",

abstract = "V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence. Although V407 Cyg likely hosts a massive accreting white dwarf, making it a candidate progenitor system for a Type Ia supernova, the dense and radially continuous circumbinary material surrounding V407 Cyg is inconsistent with observational constraints on the environments of most Type Ia supernovae.",

author = "O'brien, {Tim J.} and Eyres, {Stewart P. S.} and Bode, {Michael F.} and Osborne, {J. P.} and Page, {K. L.} and Beardmore, {A. P.} and M.R. Goad and S. Starrfield and J.-u. Ness and J. Krautter and G. Schwarz and Burrows, {D. N.} and N. Gehrels and Drake, {J. J.} and A. Evans",

year = "2010",

doi = "10.1088/0004-637X/727/2/124",

language = "English",

volume = "727",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "University of Chicago Press",

number = "2",

}

O'brien, TJ, Eyres, SPS, Bode, MF, Osborne, JP, Page, KL, Beardmore, AP, Goad, MR, Starrfield, S, Ness, J, Krautter, J, Schwarz, G, Burrows, DN, Gehrels, N, Drake, JJ & Evans, A 2010, 'Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source', The Astrophysical Journal, vol. 727, no. 2. https://doi.org/10.1088/0004-637X/727/2/124

TY - JOUR

T1 - Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source

AU - O'brien, Tim J.

AU - Eyres, Stewart P. S.

AU - Bode, Michael F.

AU - Osborne, J. P.

AU - Page, K. L.

AU - Beardmore, A. P.

AU - Goad, M.R.

AU - Starrfield, S.

AU - Ness, J.-u.

AU - Krautter, J.

AU - Schwarz, G.

AU - Burrows, D. N.

AU - Gehrels, N.

AU - Drake, J. J.

AU - Evans, A.

PY - 2010

Y1 - 2010

N2 - V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence. Although V407 Cyg likely hosts a massive accreting white dwarf, making it a candidate progenitor system for a Type Ia supernova, the dense and radially continuous circumbinary material surrounding V407 Cyg is inconsistent with observational constraints on the environments of most Type Ia supernovae.

AB - V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence. Although V407 Cyg likely hosts a massive accreting white dwarf, making it a candidate progenitor system for a Type Ia supernova, the dense and radially continuous circumbinary material surrounding V407 Cyg is inconsistent with observational constraints on the environments of most Type Ia supernovae.

U2 - 10.1088/0004-637X/727/2/124

DO - 10.1088/0004-637X/727/2/124

M3 - Article

VL - 727

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

Extensive Swift X–ray observations of nuclear burning in nova RS Oph 2006: The brightest Super–Soft Source

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