Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62...13b&link_type=abstract
Astronomy and Astrophysics, vol. 62, no. 1-2, Jan. 1978, p. 13-20. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astronomy
17
Radio Emission, Radio Sources (Astronomy), Supernova Remnants, Astronomical Maps, H Ii Regions, Hydrogen Ions, Nebulae, Point Sources, Spectrum Analysis, Thermal Radiation
Scientific paper
Direct evidence is presented which shows that the so-called Gamma Cyg radio source contains several unrelated components. The nebula nearest to the star is a typical H II region whose probable exciting star is discussed. The nonthermal part contains several long extended filaments with very steep intensity gradients. These filaments are part of a large supernova remnant. There is no physical relation between the radio components and the star, Gamma Cyg. Upper limits to the radio emission of the star are given. Attention is drawn to a point source with a peculiar spectrum.
Baars Jacob W. M.
Dickel Helene R.
Wendker Heinrich J.
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