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The predictive power of numerical simulations to study accretion and outflow in T Tauri Stars

Published online by Cambridge University Press:  20 January 2023

Ana I. Gómez de Castro Open the ORCID record for Ana I. Gómez de Castro [Opens in a new window]
Ana I. Gómez de Castro*
Affiliation:
Joint Center for Ultraviolet Astronomy, Universidad Complutense de Madrid, Avda. Puerta de Hierro s/n, 28040 Madrid, Spain email: aig@ucm.es S.D. Física de la Tierra y Astrofísica, Fac. CC Matemáticas, Plaza de Ciencias 3, 28040 Madrid, Spain
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Abstract

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T Tauri Stars (TTSs) offer a unique chance to study the physics of non-relativistic accretion engines. In this invited talk, the current status of the field is presented with special emphasis on the predictive power of the numerical simulation of magnetospheric accretion and close binary systems and its impact on astronomical observations.

Keywords

T Tauri Starsprotostellar jetsaccretion physics
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S362: The Predictive Power of Computational Astrophysics as a Discovery Tool , June 2020 , pp. 234 - 245
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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