Titlebook: JET Simulations, Experiments, and Theory; Ten Years After JETS Christophe Sauty Conference proceedings 2019 Springer Nature Switzerland AG

Parabola

ENNUI

X-Shooter Survey of Jets and Winds in T Tauri Starsh an average value of 0.07. However, considering the upper limits on the HVC, we infer a ./. ratio < 0.03 in more than 40% of sources. We argue that most of these sources might lack the physical conditions needed for an efficient magneto-centrifugal acceleration in the star-disc interaction region.

aggrieve

sleep-spindles

and among species. Obviously such broad aims cannot be met totally in a single volume, but we think we have succeeded reasonably well in providing a representat978-1-4684-6272-2978-1-4684-6270-8Series ISSN 0172-6625

音乐会

AMBI

L. Chantryand among species. Obviously such broad aims cannot be met totally in a single volume, but we think we have succeeded reasonably well in providing a representat978-1-4684-6272-2978-1-4684-6270-8Series ISSN 0172-6625

ETHER

戏法

拖网

小虫

Modeling Jet Launching from Accretion Disksuctural evolution that leads to different launching conditions over time, (ii) a new, fundamental interrelation between the disk magnetization at the launching point and the asymptotic outflow properties, (iii) the launching of jets driven by a self-generated disk dynamo magnetic field, and (iv) simulations of jets from orbiting jet sources.