activity
20182026
most citedMagnetic Field Morphology in Interstellar Clouds with the Velocity Gradient Technique

76 citations · 352 across the 22 of their papers we have counts for

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Showing astro-ph.GAShow all

19 papers · 1 filter

astro-ph.GA2026

The cosmic ray ionization rate from H3+ observations can be overestimated due to neglect of time-dependent chemistry

Ka Wai Ho, Munan Gong, Kedron Silsbee +1

The cosmic ray ionization rate (CRIR) is a key parameter governing the physical, chemical and thermal evolution of the interstellar medium. The primary technique for measuring the…

astro-ph.GA2024

Tracing magnetic field in super-Alfvenic turbulence with Gradient Technique

Ka Wai Ho, Alex Lazarian

Super-Alfvenic turbulence is important for many astrophysical objects, particularly galaxy clusters. In this paper, we explore the accuracy of Synchrotron Intensity Gradients (SIGs…

astro-ph.GA2024★ 2 cited

Statistical signatures of interstellar turbulence in dust polarization maps

Ka Wai Ho, Ka Ho Yuen, Raphael Flauger +1

We present results from a high-resolution interstellar turbulence simulation and show that it closely reproduces recent measurements. Our model captures the scaling of $EE…

astro-ph.GA2023

Sub-Alfvenic Turbulence: Magnetic to Kinetic Energy Ratio, Modification of Weak Cascade and Implications for Magnetic Field Strength Measurement

Alex Lazarian, Ka Wai HO, Ka Ho Yuen +1

We study the properties of sub-Alfvenic magnetohydrodynamic (MHD) turbulence, i.e., turbulence with Alfven Mach number , where is the velocity at the injection…

astro-ph.GA2023★ 18 cited

Nature of Striation in 21 cm Channel Maps: Velocity Caustics

Yue Hu, A. Lazarian, D. Alina +2

The alignment of striated intensity structures in thin neutral hydrogen (HI) spectroscopic channels with Galactic magnetic fields has been observed. However, the origin and nature…

astro-ph.GA2023★ 1 cited

Implementation of chemistry in the Athena++ code

Munan Gong, Ka-Wai Ho, James M. Stone +6

Chemistry plays a key role in many aspects of astrophysical fluids. Atoms and molecules are agents for heating and cooling, determine the ionization fraction, serve as observationa…