76 citations · 1.1k across the 45 of their papers we have counts for
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Parallel and Perpendicular Alignments of Velocity Gradient and Magnetic Field observed in the Molecular Clouds L1478 and L1482
Tyler Schmaltz, Yue Hu, Alex Lazarian
Star formation is a complex process that typically occurs in dense regions of molecular clouds mainly regulated by magnetic fields, magnetohydrodynamic (MHD) turbulence, and self-g…
Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
Yue Hu, Alex Lazarian
Interaction of three-dimensional magnetic fields, turbulence, and self-gravity in the molecular cloud is crucial in understanding star formation but has not been addressed so far.…
Multi-Phase Magnetic Fields in the Galaxy NGC 3627
Mingrui Liu, Yue Hu, A. Lazarian +2
Magnetic fields play an important role in the formation and evolution of a galaxy, but it is challenging to measure them by observation. Here we study the Seyfert galaxy NGC 3627's…
Turbulent Magnetic Field Amplification by the Interaction of Shock Wave and Inhomogeneous Medium
Yue Hu, Siyao Xu, James M. Stone +1
Magnetic fields on the order of 100 G observed in young supernova remnants cannot be amplified by shock compression alone. To investigate the amplification caused by turbulent d…
Magnetic Field of Molecular Gas Measured with the Velocity Gradient Technique I. Orion A
Mengke Zhao, Jianjun Zhou, Yue Hu +8
Magnetic fields play an important role in the evolution of molecular clouds and star formation. Using the Velocity Gradient Technique (VGT) model, we measured the magnetic field in…
Role of magnetic fields in fueling Seyfert nuclei
Yue Hu, Alex Lazarian, Rainer Beck +1
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 nuc…
SOFIA observations of 30 Doradus: II -- Magnetic fields and large scale gas kinematics
Le Ngoc Tram, Lars Bonne, Yue Hu +13
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…
The Velocity Statistics of Turbulent Clouds in the Presence of Gravity, Magnetic fields, Radiation, and Outflow Feedback
Yue Hu, Christoph Federrath, Siyao Xu +1
The interaction of turbulence, magnetic fields, self-gravity, and stellar feedback within molecular clouds is crucial for understanding star formation. We study the effects of self…
Probing Three-Dimensional Magnetic Fields: I -- Polarized Dust Emission
Yue Hu, A. Lazarian
Polarized dust emission is widely used to trace the plane-of-the-sky (POS) component of interstellar magnetic fields in two dimensions. Its potential to access three-dimensional ma…
Decomposing Magnetic Fields in Three Dimensions over the Central Molecular Zone
Yue Hu, A. Lazarian, Q. Daniel Wang
Measuring magnetic fields in the interstellar medium and obtaining their distribution along line-of-sight is very challenging with the traditional techniques. The Velocity Gradient…