Other
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..722y&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, April 15, 1991, p. 722-728.
Other
56
H Ii Regions, Magellanic Clouds, Supernova Remnants, Astronomical Photography, Data Reduction, H Alpha Line
Scientific paper
A new sensitive method of searching for and distinguishing supernova remnants (SNRs) from H II regions is described and applied to multifrequency radio observations and narrow-band H-alpha observations of the H II region N66 in the Small Magellanic Cloud. One SNR is identified and one SNR candidate is suggested at radio wavelengths. On an unsharp masked H-alpha plate, the H II region shows a fascinating structure which might be described by a 'champagne model'. From this and other evidence, it is suggested that giant H II regions are often associated with SNRs.
Kennicutt Robert C. Jr.
Turtle A. J.
Ye Taisheng
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