The radio spectra and physical parameters of some extended radio sources in Monoceros

Details The radio spectra and physical parameters of some extended radio sources in Monoceros The radio spectra and physical parameters of some extended radio sources in Monoceros

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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