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Pak Shing Li

Identifiers

  • name variant Pak Shing Li 0.60 · backfill

Papers (15)

  1. Magnetized interstellar molecular clouds: II. The Large-Scale Structure and Dynamics of Filamentary Molecular Clouds astro-ph.GA · 2019 · author #1
  2. Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19 astro-ph.SR · 2018 · author #7
  3. The TOP-SCOPE survey of PGCCs: PMO and SCUBA-2 observations of 64 PGCCs in the 2nd Galactic Quadrant astro-ph.GA · 2018 · author #16
  4. A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields astro-ph.GA · 2018 · author #2
  5. The Formation of Stellar Clusters in Magnetized, Filamentary Infrared Dark Clouds astro-ph.GA · 2017 · author #1
  6. ALMA reveals sequential high-mass star formation in the G9.62+0.19 complex astro-ph.GA · 2017 · author #3
  7. The CH+ Abundance in Turbulent, Diffuse Molecular Clouds astro-ph.GA · 2015 · author #3
  8. Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman Observations astro-ph.GA · 2015 · author #1
  9. Ambipolar Diffusion Heating in Turbulent Systems astro-ph.SR · 2012 · author #1
  10. A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies astro-ph.IM · 2011 · author #1
  11. Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent Enhancement astro-ph.SR · 2011 · author #1
  12. Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence astro-ph.SR · 2011 · author #11
  13. Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: II. Comparison with Observation, Clump Properties, and Scaling to Physical Units astro-ph.SR · 2010 · author #2
  14. Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: I. Turbulence Statistics astro-ph · 2008 · author #1
  15. Two regimes of Turbulent Fragmentation and the stellar IMF from Primordial to Present Day Star Formation astro-ph · 2007 · author #5

Mentions

  • 1103.5525 #11 · backfill · confidence 0.70 Pak Shing Li
  • 1007.2032 #2 · backfill · confidence 0.70 Pak Shing Li
  • 0805.0597 #1 · backfill · confidence 0.70 Pak Shing Li

Frequent Coauthors