Tidally-Induced WARPS in T-Tauri Disks - Part One - First Order Perturbation Theory

Details Tidally-Induced WARPS in T-Tauri Disks - Part One - First Order Perturbation Theory Tidally-Induced WARPS in T-Tauri Disks - Part One - First Order Perturbation Theory

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...274..291t&link_type=abstract

Astronomy and Astrophysics, Vol. 274, NO. 1/JUL(I), P. 291, 1993

Astronomy and Astrophysics

Astrophysics

32

Stars: Binaries: General, Stars: Circumstellar Matter, Stars: Flare, Stars: Pre-Main Sequence, Accretion, Accretion Disks, Celestial Mechanics

Scientific paper

We study the perturbation caused by a stellar companion on the potential of a T Tauri disk in the first-order approximation. We compute the resulting disk warp as a function of stellar and disk parameters in both cases of self-gravitating and accretion disks. We then calculate the radiative flux emitted by the warped disk, considering heating by both viscous accretion and reprocessing of stellar light. We predict that T Tauri stars with tidally warped circumstellar disks may display far-infrared and submillimetric radiative flux well in excess of that expected from flat circumstellar disks.

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