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- W32528069 abstract "The photometer (ISOPHOT) on the ESA Infrared Space Observatory (ISO) satellite was used to study the four Vega-like prototypes (Vega, β Pic, α PsA, ɛ Eri) and a set of candidate stars believed to have similar dust/debris discs. Most of the candidate stars were main sequence stars, but probably younger than Vega and ɛ Eri since they showed residual emission in the cores of their stellar spectral lines. Low resolution spectra were combined with long wavelength multi-filter photometry (between 60/μm and 200/μm) to give the spectral energy distributions for the dust/debris discs. Models suggested that the masses of the discs were between 10 −7 and 10 −4 M ⊙ (2–2000 times the mass of the moon). These were more massive than the discs around the four prototypes, but less massive than the discs around young stars such as T Tau stars." @default.
- W32528069 created "2016-06-24" @default.
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- W32528069 date "2004-01-01" @default.
- W32528069 modified "2023-09-25" @default.
- W32528069 title "ISOPHOT observations of dust discs around main sequence stars" @default.
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- W32528069 doi "https://doi.org/10.1017/s0074180900218342" @default.
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