Interstellar Matters: Neutral Hydrogen and the Galactic Magnetic Field
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/867/i=2/a=139/pdf
Reference29 articles.
1. Energy release in the solar corona from spatially resolved magnetic braids
2. Neutral Hydrogen Structures Trace Dust Polarization Angle: Implications for Cosmic Microwave Background Foregrounds
3. MAGNETICALLY ALIGNED H I FIBERS AND THE ROLLING HOUGH TRANSFORM
4. Observation of a Line in the Galactic Radio Spectrum: Radiation from Galactic Hydrogen at 1,420 Mc./sec.
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1. Gaussian Decomposition of λ21 cm H i profiles, the Critical Ionization Velocity, and the Interstellar Helium Abundance;The Astrophysical Journal;2022-08-01
2. On Interstellar Neutral Hydrogen Associated With an Hα Filament, the Critical Ionization Velocity Effect and the Origin of Filaments;IEEE Transactions on Plasma Science;2022-01
3. λ21-cm Interstellar HI Profiles, Critical Ionization Velocities, and Derived Electron Densities;IEEE Transactions on Plasma Science;2021-05
4. The physical and the geometrical properties of simulated cold H i structures;Monthly Notices of the Royal Astronomical Society;2020-12-16
5. The Role of the Critical Ionization Velocity Effect in Interstellar Space and the Derived Abundance of Helium;IEEE Transactions on Plasma Science;2020
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