High-resolution radio observations of nonthermal sources in the Rho Ophiuchus dark cloud

Details High-resolution radio observations of nonthermal sources in the Rho Ophiuchus dark cloud High-resolution radio observations of nonthermal sources in the Rho Ophiuchus dark cloud

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89..417a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, March 1984, p. 417-420. Research supported by the Iowa State University of Scien

Astronomy and Astrophysics

Astronomy

3

Astronomical Maps, Extragalactic Radio Sources, Nonthermal Radiation, Ophiuchi Clouds, Centimeter Waves, Gamma Ray Astronomy, Hydrogen Clouds, Morphology

Scientific paper

A portion of the Rho Ophiuchus dark cloud has been mapped with the VLA to investigate a possible radio counterpart to the COS-B γ-ray source 2CG353+16. The stronger two of the three sources detected have 21-cm hydrogen column densities and morphologies consistent with extragalactic sources. There is no radio counterpart to the γ-ray source detected. This negative result supports the possibility that the γ rays are emitted by the bulk mass of the cloud.

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