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Gas Dynamic Simulations of Inner Regions of Protoplanetary Disks in Young Binary Stars

Published online by Cambridge University Press:  23 April 2012

A. M. Fateeva ,
D. V. Bisikalo ,
P. V. Kaygorodov  and
A. Y. Sytov
A. M. Fateeva*
Affiliation:
Institute of Astronomy of the Russian Acad. of Sci., 48 Pyatnitskaya, Moscow, Russia
D. V. Bisikalo
Affiliation:
Institute of Astronomy of the Russian Acad. of Sci., 48 Pyatnitskaya, Moscow, Russia
P. V. Kaygorodov
Affiliation:
Institute of Astronomy of the Russian Acad. of Sci., 48 Pyatnitskaya, Moscow, Russia
A. Y. Sytov
Affiliation:
Institute of Astronomy of the Russian Acad. of Sci., 48 Pyatnitskaya, Moscow, Russia
*
*email: fateeva@inasan.ru
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We have carried out 2D and 3D numerical simulations (Kaigorodov et al 2010, Fateeva et al. 2011, Sytov et al. 2011) of accretion processes in binary T Tauri stars (TTSs) DQ Tau, UZ Tau E, V4046 Sgr, GW Ori, RoXs 42C using a finite-difference Roe-Osher-Einfeld TVD scheme. The morphology of the flow pattern for UZ Tau E is shown in Fig. 1 (left panel). The flow structure includes accretion disks surrounding the components, bow-shocks in front of both the components, a shock wave (“bridge”) between the circumstellar accretion disks and a gap containing rarefied gas in the inner part of the protoplanetary disk.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 547 - 548
Copyright
Copyright © International Astronomical Union 2012

References

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Fateeva, A. M., Bisikalo, D. V., Kaygorodov, P. V. & Sytov, A. Y. 2011, Ap&SS, 335, 125Google Scholar
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Sytov, A. Y., Kaygorodov, P. V., Fateeva, A. M. & Bisikalo, D. V. 2011, Astron. Rep., 55, 793CrossRefGoogle Scholar