Detection of the H 142-alpha line from the Barnard Loop

Details Detection of the H 142-alpha line from the Barnard Loop Detection of the H 142-alpha line from the Barnard Loop

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..149g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 149-153.

Astronomy and Astrophysics

Astronomy

9

Astronomical Spectroscopy, H Alpha Line, Hydrogen Ions, Interstellar Gas, Emission Spectra, H Ii Regions, Radial Velocity

Scientific paper

The 13-cm H142α recombination line has been observed at three positions on the Barnard Loop. The H II region parameters are derived and compared to those obtained from published optical line measurements. Optical and radio radial velocity data suggest that rotation of the Loop is occurring in the same sense as that of the associated neutral cloud, in addition to expansion.

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