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• W2023586495 abstract "Context.Far-infrared excess emission from main-sequence stars is due to dust produced by orbiting minor bodies. In these disks, larger bodies, such as planets, may also be present and the understanding of their incidence and influence currently presents a challenge." @default.
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• W2023586495 date "2008-02-14" @default.
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• W2023586495 title "q$^{mathsf{1}}$ Eridani: a solar-type star with a planet and a dust belt" @default.
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• W2023586495 doi "https://doi.org/10.1051/0004-6361:20079276" @default.
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