The Vega debris disc: A view from Herschel

B. Sibthorpe; B. Vandenbussche; J. S. Greaves; E. Pantin; G. Olofsson; B. Acke; M. J. Barlow; J. A.D.L. Blommaert; J. Bouwman; A. Brandeker; M. Cohen; W. De Meester; W. R.F. Dent; J. Di Francesco; C. Dominik; M. Fridlund; W. K. Gear; A. M. Glauser; H. L. Gomez; P. C. Hargrave; P. M. Harvey; Th Henning; A. M. Heras; M. R. Hogerheijde; W. S. Holland; R. J. Ivison; S. J. Leeks; T. L. Lim; R. Liseau; B. C. Matthews; D. A. Naylor; G. L. Pilbratt; E. T. Polehampton; S. Regibo; P. Royer; A. Sicilia-Aguilar; B. M. Swinyard; C. Waelkens; H. J. Walker; R. Wesson

doi:10.1051/0004-6361/201014574

The Vega debris disc: A view from Herschel

B. Sibthorpe
, B. Vandenbussche
, J. S. Greaves
, E. Pantin
, G. Olofsson
, B. Acke
, M. J. Barlow
, J. A.D.L. Blommaert
, J. Bouwman
, A. Brandeker
, M. Cohen
, W. De Meester
, W. R.F. Dent
, J. Di Francesco
, C. Dominik
, M. Fridlund
, W. K. Gear
, A. M. Glauser
, H. L. Gomez
, P. C. Hargrave

P. M. Harvey, Th Henning, A. M. Heras, M. R. Hogerheijde, W. S. Holland, R. J. Ivison, S. J. Leeks, T. L. Lim, R. Liseau, B. C. Matthews, D. A. Naylor, G. L. Pilbratt, E. T. Polehampton, S. Regibo, P. Royer, A. Sicilia-Aguilar, B. M. Swinyard, C. Waelkens, H. J. Walker, R. Wesson

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Abstract

We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 μm with full-width half-maximum angular resolutions of 5.6-36.9". The disc is well resolved in all bands, with the ring structure visible at 70 and 160 μm. Radial profiles of the disc surface brightness are produced, and a disc radius of 11′ (∼85 AU) is determined. The disc is seen to have a smooth structure thoughout the entire wavelength range, suggesting that the disc is in a steady state, rather than being an ephemeral structure caused by the recent collision of two large planetesimals.

Original language	English
Article number	L130
Number of pages	5
Journal	Astronomy and Astrophysics
Volume	518
DOIs	https://doi.org/10.1051/0004-6361/201014574
Publication status	Published - Jul 2010
Externally published	Yes

Keywords

instrumentation: photometers
methods: observational
stars: individual: Vega

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Sibthorpe, B., Vandenbussche, B., Greaves, J. S., Pantin, E., Olofsson, G., Acke, B., Barlow, M. J., Blommaert, J. A. D. L., Bouwman, J., Brandeker, A., Cohen, M., De Meester, W., Dent, W. R. F., Di Francesco, J., Dominik, C., Fridlund, M., Gear, W. K., Glauser, A. M., Gomez, H. L., ... Wesson, R. (2010). The Vega debris disc: A view from Herschel. Astronomy and Astrophysics, 518, Article L130. https://doi.org/10.1051/0004-6361/201014574

@article{be9458d825a94c3ea546b868709a65fa,

title = "The Vega debris disc: A view from Herschel",

abstract = "We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 μm with full-width half-maximum angular resolutions of 5.6-36.9{"}. The disc is well resolved in all bands, with the ring structure visible at 70 and 160 μm. Radial profiles of the disc surface brightness are produced, and a disc radius of 11′ (∼85 AU) is determined. The disc is seen to have a smooth structure thoughout the entire wavelength range, suggesting that the disc is in a steady state, rather than being an ephemeral structure caused by the recent collision of two large planetesimals.",

keywords = "instrumentation: photometers, methods: observational, stars: individual: Vega",

author = "B. Sibthorpe and B. Vandenbussche and Greaves, \{J. S.\} and E. Pantin and G. Olofsson and B. Acke and Barlow, \{M. J.\} and Blommaert, \{J. A.D.L.\} and J. Bouwman and A. Brandeker and M. Cohen and \{De Meester\}, W. and Dent, \{W. R.F.\} and \{Di Francesco\}, J. and C. Dominik and M. Fridlund and Gear, \{W. K.\} and Glauser, \{A. M.\} and Gomez, \{H. L.\} and Hargrave, \{P. C.\} and Harvey, \{P. M.\} and Th Henning and Heras, \{A. M.\} and Hogerheijde, \{M. R.\} and Holland, \{W. S.\} and Ivison, \{R. J.\} and Leeks, \{S. J.\} and Lim, \{T. L.\} and R. Liseau and Matthews, \{B. C.\} and Naylor, \{D. A.\} and Pilbratt, \{G. L.\} and Polehampton, \{E. T.\} and S. Regibo and P. Royer and A. Sicilia-Aguilar and Swinyard, \{B. M.\} and C. Waelkens and Walker, \{H. J.\} and R. Wesson",

year = "2010",

month = jul,

doi = "10.1051/0004-6361/201014574",

language = "English",

volume = "518",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Sibthorpe, B, Vandenbussche, B, Greaves, JS, Pantin, E, Olofsson, G, Acke, B, Barlow, MJ, Blommaert, JADL, Bouwman, J, Brandeker, A, Cohen, M, De Meester, W, Dent, WRF, Di Francesco, J, Dominik, C, Fridlund, M, Gear, WK, Glauser, AM, Gomez, HL, Hargrave, PC, Harvey, PM, Henning, T, Heras, AM, Hogerheijde, MR, Holland, WS, Ivison, RJ, Leeks, SJ, Lim, TL, Liseau, R, Matthews, BC, Naylor, DA, Pilbratt, GL, Polehampton, ET, Regibo, S, Royer, P, Sicilia-Aguilar, A, Swinyard, BM, Waelkens, C, Walker, HJ & Wesson, R 2010, 'The Vega debris disc: A view from Herschel', Astronomy and Astrophysics, vol. 518, L130. https://doi.org/10.1051/0004-6361/201014574

TY - JOUR

T1 - The Vega debris disc

T2 - A view from Herschel

AU - Sibthorpe, B.

AU - Vandenbussche, B.

AU - Greaves, J. S.

AU - Pantin, E.

AU - Olofsson, G.

AU - Acke, B.

AU - Barlow, M. J.

AU - Blommaert, J. A.D.L.

AU - Bouwman, J.

AU - Brandeker, A.

AU - Cohen, M.

AU - De Meester, W.

AU - Dent, W. R.F.

AU - Di Francesco, J.

AU - Dominik, C.

AU - Fridlund, M.

AU - Gear, W. K.

AU - Glauser, A. M.

AU - Gomez, H. L.

AU - Hargrave, P. C.

AU - Harvey, P. M.

AU - Henning, Th

AU - Heras, A. M.

AU - Hogerheijde, M. R.

AU - Holland, W. S.

AU - Ivison, R. J.

AU - Leeks, S. J.

AU - Lim, T. L.

AU - Liseau, R.

AU - Matthews, B. C.

AU - Naylor, D. A.

AU - Pilbratt, G. L.

AU - Polehampton, E. T.

AU - Regibo, S.

AU - Royer, P.

AU - Sicilia-Aguilar, A.

AU - Swinyard, B. M.

AU - Waelkens, C.

AU - Walker, H. J.

AU - Wesson, R.

PY - 2010/7

Y1 - 2010/7

N2 - We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 μm with full-width half-maximum angular resolutions of 5.6-36.9". The disc is well resolved in all bands, with the ring structure visible at 70 and 160 μm. Radial profiles of the disc surface brightness are produced, and a disc radius of 11′ (∼85 AU) is determined. The disc is seen to have a smooth structure thoughout the entire wavelength range, suggesting that the disc is in a steady state, rather than being an ephemeral structure caused by the recent collision of two large planetesimals.

AB - We present five band imaging of the Vega debris disc obtained using the Herschel Space Observatory. These data span a wavelength range of 70-500 μm with full-width half-maximum angular resolutions of 5.6-36.9". The disc is well resolved in all bands, with the ring structure visible at 70 and 160 μm. Radial profiles of the disc surface brightness are produced, and a disc radius of 11′ (∼85 AU) is determined. The disc is seen to have a smooth structure thoughout the entire wavelength range, suggesting that the disc is in a steady state, rather than being an ephemeral structure caused by the recent collision of two large planetesimals.

KW - instrumentation: photometers

KW - methods: observational

KW - stars: individual: Vega

UR - https://www.scopus.com/pages/publications/77957776160

U2 - 10.1051/0004-6361/201014574

DO - 10.1051/0004-6361/201014574

M3 - Article

AN - SCOPUS:77957776160

SN - 0004-6361

VL - 518

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - L130

ER -

The Vega debris disc: A view from Herschel

Abstract

Keywords

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