Abstract
MAPS of Carina Nebula, obtained at relatively low frequencies, have shown that most of the radiation arises from a central region and has a simple double structure, separated by about 9.4′. Gardner et al.1 studied Carina Nebula at 5 GHz, the highest frequency so far used, with the Parkes radio telescope and observed a beamwidth of 4′.
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References
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SCALISE, E., KAUFMANN, P. & ALCINA BRAZ, M. 22.2-GHz high emission nebulosities associated with the Carina Nebula central region. Nature 252, 663–664 (1974). https://doi.org/10.1038/252663a0
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DOI: https://doi.org/10.1038/252663a0
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