The Effect of Gas Drag and Radiation Pressure on Dust Around Beta Pictoris

Details The Effect of Gas Drag and Radiation Pressure on Dust Around Beta Pictoris The Effect of Gas Drag and Radiation Pressure on Dust Around Beta Pictoris

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21112405j&link_type=abstract

American Astronomical Society, AAS Meeting #211, #124.05; Bulletin of the American Astronomical Society, Vol. 39, p.954

Astronomy and Astrophysics

Astronomy

Scientific paper

The young gas-rich debris disk around Beta Pictoris is an ideal candidate to explore the likely environment of terrestrial planet formation and find new exoplanets. We are modeling the dynamics of small dust grains in this disk including the effects of gravity, radiation pressure and gas drag. Our models explore the trajectories of different size grains originating in the inner debris disk, and help the interpretation of images of the disk morphology.

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