Evidence for Residual Material in Accretion Disk Gaps: CO Fundamental Emission from the T Tauri Spectroscopic Binary DQ Tauri
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/551/i=1/a=454/pdf
Reference24 articles.
1. Dynamics of binary-disk interaction. 1: Resonances and disk gap sizes
2. Mass Flow through Gaps in Circumbinary Disks
3. The Classical T Tauri Spectroscopic Binary DQ Tau. II. Emission Line Variations with Orbital Phase.
4. Tidally Induced Gap Formation in Protostellar Disks: Gap Clearing and Suppression of Protoplanetary Growth
5. Irradiation of accretion disks around young objects. I - Near-infrared CO bands
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