Fine structure in high velocity H I gas

Details Fine structure in high velocity H I gas Fine structure in high velocity H I gas

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....54..909g&link_type=abstract

Astronomy and Astrophysics, vol. 54, no. 3, Feb. 1977, p. 909-913.

Astronomy and Astrophysics

Astrophysics

26

Astronomical Spectroscopy, Fine Structure, Hydrogen Clouds, Interstellar Gas, Gas Density, Spectral Line Width

Scientific paper

Sharp boundaries as well as small and faint concentrations associated with narrow line widths are found in the high-velocity H I complex A. The cloudlets have a product of H I mass times inverse square of distance ranging from 0.5 to 3 solar mass/sq kpc, if the gas is optically thin at 21 cm; their kinetic temperatures are less than a few hundred degrees Kelvin. They could provide the missing link between the H I high-velocity clouds and anomalous-velocity clouds observed in other spectral domains.

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