The HI column density as a function of position in the southern sky

Details The HI column density as a function of position in the southern sky The HI column density as a function of position in the southern sky

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aujpa..47....1h&link_type=abstract

Australian Journal of Physics, Astrophysical Supplement, no. 47, Sept. 1979, p. 1-58. NSF-supported research.

Astronomy and Astrophysics

Astronomy

92

Gas Density, Hydrogen Clouds, Tables (Data), Atom Concentration, Hydrogen Atoms, Ultraviolet Astronomy, X Ray Astronomy

Scientific paper

An H I survey of the southern sky (delta not more than -30 deg) was made with the Parkes 18-m telescope, covering a velocity range of 448 km/s with 64 channels. This paper presents tables giving H I column densities for the LSR velocity ranges -50 to +50 km/s and -100 to +100 km/s for delta not more than -30 deg and absolute value of b not less than 10 deg.

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