Observations of the radio source G6.6-0.1 positionally coincident with the W28 SNR

Details Observations of the radio source G6.6-0.1 positionally coincident with the W28 SNR Observations of the radio source G6.6-0.1 positionally coincident with the W28 SNR

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90..310a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, Feb. 1985, p. 310-314. Research supported by Iowa State University of Science an

Astronomy and Astrophysics

Astronomy

6

H Alpha Line, Radio Sources (Astronomy), Supernova Remnants, Astronomical Maps, Continuous Spectra, Hydrogen Clouds, Thermal Emission

Scientific paper

This paper reports scaled-array continuum and H76α line
observations of the radio source G 6.6-0.1 which is positioned at the
center of the W28 SNR. The source exhibits a bright core surrounded by
extended emission which appears organized into arcs and wisps. G 6.6-0.1
is interpreted as a compact H II region with a unique morphology.

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