Observations at 8.87 GHz in the Milky Way near L = 333 deg

Details Observations at 8.87 GHz in the Milky Way near L = 333 deg Observations at 8.87 GHz in the Milky Way near L = 333 deg

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.189..413m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 189, Nov. 1979, p. 413-419.

Astronomy and Astrophysics

Astronomy

11

Hydrogen Recombinations, Microwave Spectra, Milky Way Galaxy, Radio Astronomy, Supernova Remnants, Continuous Radiation, Continuous Spectra, Electron Energy, Galactic Structure, Hydrogen Clouds, Radial Velocity, Radio Sources (Astronomy)

Scientific paper

A region of sky in the constellation Norma, near 333 deg galactic longitude, has been observed in the radio continuum and for the presence of hydrogen recombination lines at a frequency of 8.87 GHz with a telescope beam having a HPBW of 2.5 arcmin. The results show that most of the large number (at least 64) of sources in the region form part of a spiral arm at a distance of approximately 3.7 kpc from the sun.

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