Hints for Small Disks around Very Low Mass Stars and Brown Dwarfs

Hints for Small Disks around Very Low Mass Stars and Brown Dwarfs

The properties of disks around brown dwarfs and very low mass stars (hereafter VLMOs) provide important boundary conditions on the process of planet formation and inform us about the numbers and masses of planets than can form in this regime. We use the Herschel Space Observatory PACS spectrometer t...

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Bibliographic Details
Main Authors: Hendler, Nathanial P., Mulders, Gijs D., Pascucci, Ilaria, Greenwood, Aaron, Kamp, Inga, Henning, Thomas, Menard, Francois, Dent, William R. F., Evans, Neal J., II
Other Authors: Univ Arizona, Lunar & Planetary Lab
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
brown dwarfs
circumstellar matter
protoplanetary disks
Online Access:http://hdl.handle.net/10150/624452
http://arizona.openrepository.com/arizona/handle/10150/624452

Internet

http://hdl.handle.net/10150/624452
http://arizona.openrepository.com/arizona/handle/10150/624452

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