H I 21 CM line observations at low galactic latitudes in the Southern Hemisphere

Details H I 21 CM line observations at low galactic latitudes in the Southern Hemisphere H I 21 CM line observations at low galactic latitudes in the Southern Hemisphere

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26as...41..121b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 41, July 1980, p. 121-128.

Astronomy and Astrophysics

Astronomy

2

Astronomical Maps, Astronomical Spectroscopy, Hydrogen Atoms, Interstellar Gas, Milky Way Galaxy, Neutral Gases, Brightness Temperature, Centimeter Waves, Microwave Spectra, Radio Astronomy, Southern Hemisphere

Scientific paper

An H I survey from 21 cm observations on a regular grid in the region defined by 220° ≤ l ≤ 269°, -10° ≤ b ≤ 2° is described in this paper. The observations were done with the IAR 30 m dish. Contour maps for the brightness temperature are presented in the form of b-V plots at constant l, every 2° from 220° to 240° and every 1° from 240° to 269°, and l-V plots at constant b every 1° from -10° to +2°.

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