WSRT observations of radio sources in the galactic plane near L = 54 deg

Details WSRT observations of radio sources in the galactic plane near L = 54 deg WSRT observations of radio sources in the galactic plane near L = 54 deg

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986japa....7..105v&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 7, June 1986, p. 105-112.

Astronomy and Astrophysics

Astronomy

6

Astronomical Maps, Milky Way Galaxy, Radio Sources (Astronomy), Stellar Structure, Supernova Remnants, Centimeter Waves, Hydrogen Clouds, Interstellar Matter, Radiant Flux Density, Spectral Energy Distribution, Stellar Spectrophotometry

Scientific paper

A radio continuum map of 1.5 deg region in the galactic plane near l = 54 deg is presented at 49 cm with a resolution of 100 arcsec x 200 arcsec. The shell source G 54.4 - 0.3 has the characteristics of a supernova remnant while the second large ring structure G 53.9 + 0.3 is a H II ring consisting of W 52 and several small-diameter thermal sources. One of the twelve small-diameter sources (G 54.73 + 0.61) has a spectral index about -1.6.

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