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Cited article:

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 139 (6) 2410 (2010)
https://doi.org/10.1088/0004-6256/139/6/2410