@inproceedings{0a8a09184b2a4d598199f0019e8b26ce,
title = "Modelling the Accretion on Young Stars, Recent Results and Perspectives",
abstract = "Despite intense observational work, the stellar accretion process is insufficiently constrained, and consequently the details in the exchange of mass and momentum between the proto-star and its accretion disk remain approximate. We focus here on 1D simulations of accretion columns falling onto a stellar chromosphere. After the description of the method used for the radiative hydrodynamics, we first describe the mutual feedback between a dynamically heated chromosphere and the accretion process and the coupling between radiation and matter. Perspectives to this work will finally be presented.",
author = "{de S{\'a}}, L. and C. Stehl{\'e} and Chi{\`e}ze, {J. P.} and I. Hubeny and T. Lanz and S. Colombo and L. Ibgui and S. Orlando",
note = "Funding Information: These studies have been funded by the French “Programme National de Physique Stellaire” of INSU, the French Italian cooperation program PICS 6838 “Physics of Mass Accretion Processes in Young Stellar Objects”, the Observatoire de Paris and the LABEX PLAS@PAR (ANR-11-IDEX-0004-02). Publisher Copyright: {\textcopyright} 2019, Springer Nature Switzerland AG.; Workshop on JET Simulations, Experiments, and Theory, JETSET 2018 ; Conference date: 22-05-2018 Through 24-05-2018",
year = "2019",
doi = "10.1007/978-3-030-14128-8_4",
language = "English (US)",
isbn = "9783030141271",
series = "Astrophysics and Space Science Proceedings",
publisher = "Springer Netherlands",
pages = "29--35",
editor = "Christophe Sauty",
booktitle = "JET Simulations, Experiments, and Theory - 10 Years After JETSET. What Is Next?, 2018",
}