The velocities of 6cm recombination line emission originating near the galactic nucleus

Details The velocities of 6cm recombination line emission originating near the galactic nucleus The velocities of 6cm recombination line emission originating near the galactic nucleus

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasau...3..150g&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 11th, Clayton, Victoria, Australia, May 30-June 1, 1977.) Astronomic

Astronomy and Astrophysics

Astronomy

10

Galactic Nuclei, Line Spectra, Milky Way Galaxy, Radiative Recombination, Electron Energy, Electron Radiation, Electron Scattering, H Ii Regions, Hydrogen Ions, Supernovae

Scientific paper

The kinematics of the H II regions near the center of the galaxy are investigated with a beamwidth of 4.5 minutes of arc, and are found to have an ordered motion. Electron temperatures of the regions are evaluated as a clue to a possible mechanism of continuum radiation. It is also suggested that the mechanism may be nonthermal, i.e., supersonic motion producing line emission through collisions. Also considered is the possibility that the region may have resulted from a supernova explosion.

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