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- W1569329253 abstract "Our efficient numerical approach has been applied to modeling the asymmetric circumstellar dust disk around β Pictoris as observed with the HST/STIS. We present a new model on the origin of the warping of the β Pic disk. We suggest that the observed warp is formed by the gravitational influence of a planet with a mass of about 10 masses of Earth, at a distance of 70 AU, and a small inclination (∽ 2.5°) of the planetary orbit to the main dust disk. Results of our modeling are compared with the STIS observations." @default.
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- W1569329253 date "2004-01-01" @default.
- W1569329253 modified "2023-10-16" @default.
- W1569329253 title "Indicator of Exo-Solar Planet(s) in the Circumstellar Disk Around β Pictoris" @default.
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- W1569329253 doi "https://doi.org/10.1017/s0074180900218160" @default.
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