Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-07-18
Astrophys.J.593:L117-L120,2003
Astronomy and Astrophysics
Astrophysics
Accepted in ApJ Letters - 4 pages - 2 figures
Scientific paper
10.1086/378285
We propose that the large photometric variations of KH15D are due to an eclipsing swarm of solid particles trapped in giant gaseous vortex rotating at \~0.2 AU from the star. The efficiency of the capture-in-vortex mechanism easily explains the observed large optical depth. The weaker opacity at mid-eclipse is consistent with a size segregation of the particles toward the center of the vortex. This dusty structure must extend over ~1/3 of an orbit to account for the long eclipse duration. The estimated size of the trapped particles is found to range from 1 to 10cm, consistent with the gray extinction of the star. The observations of KH15D support the idea that giant vortices can grow in circumstellar disks and play a central role in planet formation.
Barge Pierre
Viton Maurice
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