Detection of the H200-beta line in the direction of the galactic centre

Details Detection of the H200-beta line in the direction of the galactic centre Detection of the H200-beta line in the direction of the galactic centre

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59l..31s&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 3, Aug. 1977, p. L31, L32.

Astronomy and Astrophysics

Astrophysics

5

Galactic Radiation, H Beta Line, Galactic Nuclei, H Ii Regions, Line Spectra, Milky Way Galaxy, Spectrum Analysis

Scientific paper

The H200-beta line in the direction of Sgr A has been detected, with approximately the LTE intensity. This contradicts two published upper limits which had implied extreme physical conditions in the line-emitting gas. The observations can now be interpreted simply in terms of line-of-sight low-density H II regions, similar to those seen in other directions.

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