Low-latitude radio continuum structure in the fourth galactic quadrant

Details Low-latitude radio continuum structure in the fourth galactic quadrant Low-latitude radio continuum structure in the fourth galactic quadrant

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.219....1j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 219, March 1, 1986, p. 1-12. Research supported by Rhod

Astronomy and Astrophysics

Astronomy

6

Continuous Spectra, Galactic Radio Waves, Milky Way Galaxy, Radio Astronomy, Astronomical Coordinates, Astronomical Maps, Spectrum Analysis, Supernova Remnants

Scientific paper

A number of new galactic continuum emission features have been found at
low latitudes between longitudes 310° and 5°. These sources are
in the form of loops, spurs and arcs which have angular dimensions
between 2 and 6°. An attempt is made to classify each of the new
sources, and in some cases determine their distance from the Sun.

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