Morphology of gas flow during collision of accretion disks in a T Tauri type binary with elliptic orbit
Abstract
We present the results of numerical simulation of interacting accretion disks in a T Tauri type binary with elliptic orbit. Using these results we study structure and evolution of the system of shock waves in accretion disks and between them. Finally we discuss the possibility of bringing up an analytical model for accretion disk interaction.
- Publication:
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INASAN Science Reports
- Pub Date:
- December 2020
- DOI:
- 10.51194/INASAN.2020.5.6.004
- Bibcode:
- 2020INASR...5..327S
- Keywords:
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- binary stars;
- stellar masses