Abstract
We present Herschel PACS 100 and 160 μm observations of the solar-type stars α Men, HD 88230 and HD 210277, which form part of the FGK stars sample of the Herschel open time key programme (OTKP) DUNES (DUst around NEarby S tars). Our observations show small infrared excesses at 160 μm for all three stars. HD 210277 also shows a small excess at 100 μm, while the 100 μm fluxes of α Men and HD 88230 agree with the stellar photospheric predictions. We attribute these infrared excesses to a new class of cold, faint debris discs. Both ? Men and HD 88230 are spatially resolved in the PACS 160 μm images, while HD 210277 is point-like at that wavelength. The projected linear sizes of the extended emission lie in the range from ∼115 to ≤250 AU. The estimated black body temperatures from the 100 and 160 ?m fluxes are ≈22 K, and the fractional luminosity of the cold dust is L dust/Lz.ast ∼ 10?6, close to the luminosity of the solar-system's Kuiper belt. These debris discs are the coldest and faintest discs discovered so far around mature stars, so they cannot be explained easily invoking "classical" debris disc models. © 2011 ESO.
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Eiroa, C., Marshall, J. P., Mora, A., Krivov, A. V., Montesinos, B., Absil, O., … Wolf, S. (2011). Herschel discovery of a new class of cold, faint debris discs. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/201117797
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