Spectroscopy of the B-gamma line in the Galactic center

Details Spectroscopy of the B-gamma line in the Galactic center Spectroscopy of the B-gamma line in the Galactic center

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86..561n&link_type=abstract

Astronomical Journal, vol. 86, Apr. 1981, p. 561-564. NASA-NSF-supported research.

Astronomy and Astrophysics

Astronomy

14

Astronomical Spectroscopy, Galactic Nuclei, Line Spectra, Milky Way Galaxy, Emission Spectra, Hydrogen Clouds, Hydrogen Recombinations, Ionized Gases

Scientific paper

Spectra of the B-gamma recombination line of hydrogen in the Galactic center show that the line has central velocities and shapes similar to those reported previously for the Ne II line. Observations are made at 10 positions within the infrared cluster of the Galactic center with a circular diaphragm of diameter 5 arcsec and with a spectral resolution of approximately 85 km/sec. The spectra confirm that the ionized gas in the Galactic center is distributed in discrete clouds.

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