Observations of 85-alpha recombination lines from W48

Details Observations of 85-alpha recombination lines from W48 Observations of 85-alpha recombination lines from W48

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jrasc..71..377m&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 71, Oct. 1977, p. 377-385.

Astronomy and Astrophysics

Astronomy

2

Hydrogen Clouds, Hydrogen Recombinations, Line Spectra, Radio Astronomy, Radio Sources (Astronomy), Astronomical Coordinates, Electron Energy, Radial Velocity, Radiant Flux Density, Radio Spectra

Scientific paper

Hydrogen 85-alpha recombination lines have been detected from all three
components of the source W48, including a component previously suggested
to be nonthermal. A continuum map with a resolution of 2.7 arcmin is
presented. It is suggested that W48 is part of a larger molecular cloud
which reaches as far west as the neighboring supernova remnant W44.

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