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...

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Veröffentlicht in:	arXiv.org 2016-03
Hauptverfasser:	Meng, Huan Y A, Plavchan, Peter, Rieke, George H, Cody, Ann Marie, Güth, Tina, Stauffer, John, Covey, Kevin, Carey, Sean, Ciardi, David, Duran-Rojas, Maria C, Gutermuth, Robert A, Morales-Calderón, María, Rebull, Luisa M, Watson, Alan M
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Adaptive optics Constraint modelling Magnetospheres Mapping Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Star & galaxy formation Star formation Stellar surfaces Sublimation T Tauri stars Travel time
Online-Zugang:	Volltext
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