8 citations · 8 across the 4 of their papers we have counts for
4 papers · 1 filter
modeling of Galactic dust polarized CMB foreground
Alexei G. Kritsuk, Ka Wai Ho, Ka Ho Yuen +1
We present the analysis of high-resolution synthetic dust polarization maps derived from large-scale simulations of magnetized multiphase interstellar turbulence carried out with t…
Applying the Velocity Gradient Technique in NGC 1333: Comparison with Dust Polarization Observations
Archana Soam, Ka Ho Yuen, Ian Stephens +3
Magnetic fields (B-fields) are ubiquitous in the interstellar medium (ISM), and they play an essential role in the formation of molecular clouds and subsequent star formation. Howe…
The stable "Unstable Natural Media" due to the presence of turbulence
Ka Wai Ho, Ka Ho Yuen, Alex Lazarian
The term "unstable neutral media" (UNM) has traditionally been used to describe the transient phase formed between the warm and cold neutral hydrogen (HI) phases and has not been t…
Neutral hydrogen filaments in interstellar media: Are they physical?
Ka Ho Yuen, Ka Wai Ho, Chi Yan Law +1
The trending term "filament" is extensively used in the interstellar medium (ISM) and the star formation community, and is believed to be one of the most important objects that gau…