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- W2153226930 abstract "We report on a first attempt to detect Vega's disk through optical scattered light by using linear photopolarimetry. Polarization measurements on the aureole of Vega were carried out between 7 00 and 30 00 from the star with a 10 00 diameter hole and down to polarization level of 10 4 . No signal reliably attributable to circumstellar dust was detected, and an upper limit to the polarized surface brightness of the disk is derived. This upper limit for Vega's disk is about 200 times lower than the polarized brightness observed around Pic, at an angular offset of 15 00 from the stars." @default.
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- W2153226930 date "1998-09-01" @default.
- W2153226930 modified "2023-09-23" @default.
- W2153226930 title "AN ATTEMPT TO DETECT THE DUST DISK OF VEGA BY PHOTOPOLARIMETRY, AND CONSTRAINTS ON THE GRAIN SIZE" @default.
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