Millimeter Spectral Indices and Dust Trapping By Planets in Brown Dwarf Disks

Millimeter Spectral Indices and Dust Trapping By Planets in Brown Dwarf Disks

Disks around brown dwarfs (BDs) are excellent laboratories to study the first steps of planet formation in cold and low-mass disk conditions. The radial-drift velocities of dust particles in BD disks higher than in disks around more massive stars. Therefore, BD disks are expected to be more depleted...

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Bibliographic Details
Main Authors: Pinilla, P., Quiroga-Nuñez, L. H., Benisty, M., Natta, A., Ricci, L., Henning, Th., van der Plas, G., Birnstiel, T., Testi, L., Ward-Duong, K.
Other Authors: Univ Arizona, Dept Astron, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
brown dwarfs
circumstellar matter
planets and satellites: formation
protoplanetary disks
Online Access:http://hdl.handle.net/10150/625749
http://arizona.openrepository.com/arizona/handle/10150/625749

Internet

http://hdl.handle.net/10150/625749
http://arizona.openrepository.com/arizona/handle/10150/625749

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