PHOTO-REVERBERATION MAPPING OF A PROTOPLANETARY ACCRETION DISK AROUND A T TAURI STAR
Theoretical models and spectroscopic observations of newborn stars suggest that protoplantary disks have an inner "wall" at a distance set by the disk interaction with the star. Around T Tauri stars, the size of this disk hole is expected to be on a 0.1 au scale that is unresolved by curre...
Main Authors: | , , , , , , , , , , , , , |
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Other Authors: | |
Language: | en |
Published: |
IOP PUBLISHING LTD
2016
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/621264 http://arizona.openrepository.com/arizona/handle/10150/621264 |