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

Cyfadran Cyfrifiadureg, Peirianneg a Gwyddoniaeth

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

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V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence.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.

Iaith wreiddiol	Saesneg
Cyfnodolyn	The Astrophysical Journal
Cyfrol	727
Rhif cyhoeddi	2
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1088/0004-637X/727/2/124
Statws	Cyhoeddwyd - 2010

Mynediad at Ddogfen

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

Dyfynnu hyn

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abstract = "V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence.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, cyfrol. 727, rhif 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

SN - 0004-637X

VL - 727

JO - The Astrophysical Journal

JF - The Astrophysical Journal

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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