Ionized gas in the inner Galaxy - The 3 kiloparsec arm

Details Ionized gas in the inner Galaxy - The 3 kiloparsec arm Ionized gas in the inner Galaxy - The 3 kiloparsec arm

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...356..156c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 356, June 10, 1990, p. 156-159. Research supported by CONICET.

Astronomy and Astrophysics

Astrophysics

2

H Ii Regions, Interstellar Gas, Ionized Gases, Milky Way Galaxy, Emission Spectra, Galactic Structure, Radio Emission, Recombination Reactions

Scientific paper

New detections are reported for the H166-alpha recombination line at high velocity in four directions of the inner Galaxy located at galactocentric distance R(G) less than 4 kpc. The distribution of the ionized gas in the inner Galaxy is analyzed. It is found that low-density ionized gas is located along the 3 kpc arm. The presence of this gas argues that the H II region are in a latest stage of development.

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