Other
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..555d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 186, Feb. 1979, p. 555-562.
Other
10
Abundance, Astronomical Spectroscopy, Line Spectra, Supernova Remnants, H Ii Regions, Magellanic Clouds, Nitrogen, Spectrum Analysis, Spiral Galaxies, Sulfur
Scientific paper
Spectral data are presented confirming the classification of three nebulae in M33 as supernova remnants, a result supported by available radio data. A comparison with other supernova remnants and model calculations has been made. Several lines of evidence indicate a nitrogen abundance slightly lower than that in the Galaxy, and consistent with the abundance trends in H II regions at similar radial distance in M33 reported by Searle and Smith. Discrepancies still exist, however, between the observed spectra and model calculations.
Clark David H.
Danziger Ivan John
Dodorico Sandro
Murdin P. G.
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