22-GHz continuum observations of the Carina nebula

Details 22-GHz continuum observations of the Carina nebula 22-GHz continuum observations of the Carina nebula

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..716t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, April 15, 1991, p. 716-721.

Astronomy and Astrophysics

Astronomy

10

Nebulae, Open Clusters, Peculiar Stars, Radio Astronomy, Radio Sources (Astronomy), Nonthermal Radiation, Radio Telescopes, Supernova Remnants, Thermal Emission

Scientific paper

The Carina nebula was observed at 22 GHz using the 13.7-m Itapetinga Radio Telescope. The radio structure of the Carina region shows three lobes running perpendicular to the Galactic plane, suggesting a large-scale configuration, such as separate spiral arms, to explain the radio features. In addition, a spectral index survey was carried out over the nebula which indicated several nonthermal regions. They were interpreted as due to an old supernova remnant in front of the nebula.

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