Magneto-thermal disk winds from protoplanetary disks
The global evolution and dispersal of protoplanetary disks (PPDs) are governed by disk
angular-momentum transport and mass-loss processes. Recent numerical studies suggest …
angular-momentum transport and mass-loss processes. Recent numerical studies suggest …
Molecular outflows in low-and high-mass star forming regions
HG Arce, D Shepherd, F Gueth, CF Lee… - arXiv preprint astro-ph …, 2006 - arxiv.org
We review the known properties of molecular outflows from low-and high-mass young stars.
General trends among outflows are identified, and the most recent studies on the …
General trends among outflows are identified, and the most recent studies on the …
Global evolution of an accretion disk with a net vertical field: coronal accretion, flux transport, and disk winds
Z Zhu, JM Stone - The Astrophysical Journal, 2018 - iopscience.iop.org
We report results from global ideal MHD simulations that study thin accretion disks (with
thermal scale height H/R= 0.1 and 0.05) threaded by net vertical magnetic fields. Our …
thermal scale height H/R= 0.1 and 0.05) threaded by net vertical magnetic fields. Our …
Disk winds, jets, and outflows: theoretical and computational foundations
RE Pudritz, R Ouyed, C Fendt… - arXiv preprint astro-ph …, 2006 - arxiv.org
We review advances in the theoretical and computational studies of disk winds, jets and
outflows including: the connection between accretion and jets, the launch of jets from …
outflows including: the connection between accretion and jets, the launch of jets from …
Launching of conical winds and axial jets from the disc–magnetosphere boundary: axisymmetric and 3D simulations
MM Romanova, GV Ustyugova… - Monthly Notices of …, 2009 - academic.oup.com
We investigate the launching of outflows from the disc–magnetosphere boundary of slowly
and rapidly rotating magnetized stars using axisymmetric and exploratory 3D …
and rapidly rotating magnetized stars using axisymmetric and exploratory 3D …
The formation of massive stars
H Beuther, EB Churchwell, CF McKee… - arXiv preprint astro-ph …, 2006 - arxiv.org
Massive stars have a profound influence on the Universe, but their formation remains poorly
understood. We review the current status of observational and theoretical research in this …
understood. We review the current status of observational and theoretical research in this …
[图书][B] Magnetohydrodynamics in binary stars
CG Campbell - 1997 - Springer
Since the publication of the first edition, the area of magnetic fields in binary stars has
continued to expand. The number of known AM Herculis binaries has more than doubled in …
continued to expand. The number of known AM Herculis binaries has more than doubled in …
Resistive relativistic MHD simulations of astrophysical jets
G Mattia, L Del Zanna, M Bugli, A Pavan… - Astronomy & …, 2023 - aanda.org
Aims. The main goal of the present paper is to provide the first systematic numerical study of
the propagation of astrophysical relativistic jets, in the context of high-resolution, shock …
the propagation of astrophysical relativistic jets, in the context of high-resolution, shock …
Synchrotron radiation of self-collimating relativistic magnetohydrodynamic jets
The goal of this paper is to derive signatures of synchrotron radiation from state-of-the-art
simulation models of collimating relativistic magnetohydrodynamic (MHD) jets featuring a …
simulation models of collimating relativistic magnetohydrodynamic (MHD) jets featuring a …
Jet launching in resistive GR-MHD black hole–accretion disk systems
Q Qian, C Fendt, C Vourellis - The Astrophysical Journal, 2018 - iopscience.iop.org
We investigate the launching mechanism of relativistic jets from black hole sources, in
particular the strong winds from the surrounding accretion disk. Numerical investigations of …
particular the strong winds from the surrounding accretion disk. Numerical investigations of …