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Galactic Neutral Hydrogen Emission Profile Structure

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Gerrit L. Verschuur1 and Anthony L. Peratt2,3

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[1]

A Pervasive Broad Component in H I Emission Line Profiles: Temperature, Turbulence, or a Helium Signature?

G. L. Verschuur and J. T. Schmelz  The Astronomical Journal 2010  139 2410
IOPscience 
[2]

On the Apparent Associations Between Interstellar Neutral Hydrogen Structure and (WMAP) High-frequency Continuum Emission

Gerrit L. Verschuur  The Astrophysical Journal 2010  711 1208
IOPscience 
[3]

Gerrit L. Verschuur  IEEE Transactions on Plasma Science 2007  35 759
CrossRef 
[4]

Valentin A. Rantsev-Kartinov  IEEE Transactions on Plasma Science 2007  35 767
CrossRef 
[5]

Gaussian decomposition of Hi surveys

U. Haud and P. M. W. Kalberla  Astronomy and Astrophysics 2007  466 555
CrossRef 
[6]

Interstellar Neutral Hydrogen Emission Profile Structure

Gerrit L. Verschuur  The Astronomical Journal 2004  127 394
IOPscience 
[7]

A review of critical ionization velocity

Shu T. Lai  Reviews of Geophysics 2001  39 471
CrossRef 
[8]

Observation of the CIV effect in interstellar clouds: a speculation on the physical mechanism for their existence

A.L. Peratt and G.L. Verschuur  IEEE Transactions on Plasma Science 2000  28 2122
CrossRef 
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