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Recent progress in theory and observational study of dust grain alignment and rotational disruption in star-forming regions
Modern understanding of dust astrophysics reveals that radiative torques (RATs) arising
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
from the radiation–dust interaction can induce two fundamental effects: grain alignment and …
Magnetic fields in star formation: from clouds to cores
In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …
play throughout the star formation process, gained through observations and simulations of …
Synchrotron intensity gradient revealing magnetic fields in galaxy clusters
Magnetic fields and their dynamical interplay with matter in galaxy clusters contribute to the
physical properties and evolution of the intracluster medium. However, the current …
physical properties and evolution of the intracluster medium. However, the current …
Superdiffusion of cosmic rays in compressible magnetized turbulence
Owing to the complexity of turbulent magnetic fields, modelling the diffusion of cosmic rays is
challenging. Based on the current understanding of anisotropic magnetohydrodynamic …
challenging. Based on the current understanding of anisotropic magnetohydrodynamic …
Probing three-dimensional magnetic fields: II–an interpretable Convolutional Neural Network
Observing 3D magnetic fields, including orientation and strength, within the interstellar
medium is vital but notoriously difficult. However, recent advances in our understanding of …
medium is vital but notoriously difficult. However, recent advances in our understanding of …
Turbulent magnetic field amplification by the interaction of a shock wave and inhomogeneous medium
Magnetic fields of the order of 100 μG observed in young supernova remnants cannot be
amplified by shock compression alone. To investigate the amplification caused by a …
amplified by shock compression alone. To investigate the amplification caused by a …
Role of magnetic fields in fueling Seyfert nuclei
Molecular gas is believed to be the fuel for star formation and nuclear activity in Seyfert
galaxies. To explore the role of magnetic fields in funneling molecular gas into the nuclear …
galaxies. To explore the role of magnetic fields in funneling molecular gas into the nuclear …
Nature of striation in 21 cm channel Maps: velocity caustics
The alignment of striated intensity structures in thin neutral hydrogen (H i) spectroscopic
channels with Galactic magnetic fields has been observed. However, the origin and nature …
channels with Galactic magnetic fields has been observed. However, the origin and nature …
Sofia observations of 30 doradus. ii. magnetic fields and large-scale gas kinematics
The heart of the Large Magellanic Cloud, 30 Doradus, is a complex region with a clear core-
halo structure. Feedback from the stellar cluster R136 has been shown to be the main …
halo structure. Feedback from the stellar cluster R136 has been shown to be the main …
Gradient Technique Theory: Tracing magnetic field and obtaining magnetic field strength
The gradient technique is a promising tool with theoretical foundations based on the
fundamental properties of MHD turbulence and turbulent reconnection. Its various …
fundamental properties of MHD turbulence and turbulent reconnection. Its various …