Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..43..135g&link_type=abstract
Astrophysics and Space Science, vol. 43, Aug. 1976, p. 135-143. Research supported by the Science Research Council.
Astronomy and Astrophysics
Astronomy
4
Radio Sources (Astronomy), Radio Spectra, Supernova Remnants, Astronomical Maps, Astronomical Models, H Ii Regions, Nebulae, Radio Astronomy, Rosette Shapes, Spectrum Analysis
Scientific paper
The radio spectra of the Rosette Nebula, the source S280, and the Monoceros Nebulosity are established over a wide range of frequencies. The radio spectra of the Rosette Nebula and S280 show a typical thermal shape. Physical parameters of both H II regions are derived by adopting a spherical model. The radio spectrum of the Monoceros Nebulosity shows a nonthermal shape (spectral index -0.66) but the exact nature of the object is not clear. Assuming it is a supernova remnant, some of its physical characteristics are estimated.
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