Resolving debris discs in the far-infrared: Early highlights from the DEBRIS survey

We present results from the earliest observations of DEBRIS, a Herschel key programme to conduct a volume- and flux-limited survey for debris discs in A-type through M-type stars. PACS images (from chop/nod or scan-mode observations) at 100 and 160 μm are presented toward two A-type stars and one F-...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2010-07, Vol.518 (1), p.L135
Hauptverfasser: Matthews, B. C., Sibthorpe, B., Kennedy, G., Phillips, N., Churcher, L., Duchêne, G., Greaves, J. S., Lestrade, J.-F., Moro-Martin, A., Wyatt, M. C., Bastien, P., Biggs, A., Bouvier, J., Butner, H. M., Dent, W. R. F., Di Francesco, J., Eislöffel, J., Graham, J., Harvey, P., Hauschildt, P., Holland, W. S., Horner, J., Ibar, E., Ivison, R. J., Johnstone, D., Kalas, P., Kavelaars, J., Rodriguez, D., Udry, S., van der Werf, P., Wilner, D., Zuckerman, B.
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container_issue 1
container_start_page L135
container_title Astronomy and astrophysics (Berlin)
container_volume 518
creator Matthews, B. C.
Sibthorpe, B.
Kennedy, G.
Phillips, N.
Churcher, L.
Duchêne, G.
Greaves, J. S.
Lestrade, J.-F.
Moro-Martin, A.
Wyatt, M. C.
Bastien, P.
Biggs, A.
Bouvier, J.
Butner, H. M.
Dent, W. R. F.
Di Francesco, J.
Eislöffel, J.
Graham, J.
Harvey, P.
Hauschildt, P.
Holland, W. S.
Horner, J.
Ibar, E.
Ivison, R. J.
Johnstone, D.
Kalas, P.
Kavelaars, J.
Rodriguez, D.
Udry, S.
van der Werf, P.
Wilner, D.
Zuckerman, B.
description We present results from the earliest observations of DEBRIS, a Herschel key programme to conduct a volume- and flux-limited survey for debris discs in A-type through M-type stars. PACS images (from chop/nod or scan-mode observations) at 100 and 160 μm are presented toward two A-type stars and one F-type star: β Leo, β UMa and η Corvi. All three stars are known disc hosts. Herschel spatially resolves the dust emission around all three stars (marginally, in the case of β UMa), providing new information about discs as close as 11 pc with sizes comparable to that of the Solar System. We have combined these data with existing flux density measurements of the discs to refine the SEDs and derive estimates of the fractional luminosities, temperatures and radii of the discs.
doi_str_mv 10.1051/0004-6361/201014667
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subjects Astronomy
Astrophysics
circumstellar matter
Earth, ocean, space
Exact sciences and technology
infrared: stars
Sciences of the Universe
stars: individual: β Leo
stars: individual: β UMa
stars: individual: η Corvi
title Resolving debris discs in the far-infrared: Early highlights from the DEBRIS survey
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