Abstract
ABSTRACT This note reports the identification of 11 supernova remnant (SNR) candidates in a field 22 arcmin in diameter centered on M33, excluding the nuclear region. The SNR candidates were distinguished from H II regions on the basis of optical appearance on direct red plates and the presence of strong forbidden S II emission relative to (H-alpha + forbidden N II) emission. Finding charts and essential data on the SNR candidates are provided, and some properties of the individual objects are discussed.
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