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II.</title><shortName>J/PASP/111/685</shortName><identifier>ivo://CDS.VizieR/J/PASP/111/685</identifier><altIdentifier>doi:10.26093/cds/vizier.61110685</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hodge P.W.</name></creator><creator><name>Balsley J.</name></creator><creator><name>Wyder T.K.</name></creator><creator><name>Skelton B.P.</name></creator><date role="Updated">2025-09-09T14:12:36Z</date><date role="Created">2003-11-10T10:07:11Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>h-ii-regions</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>We have identified a total of 1272 newly recognized emission regions in M33. Combined with the previously cataloged total of 1066 H II regions and supernova remnants, this brings M33's total to 2338 emission regions. This paper provides photometry of the new objects in H{alpha}, which is combined with data from previous catalogs to produce a global H II region luminosity function (corrected for incompleteness) that reaches a faint luminosity limit of 2x10^34^ergs/s and shows a broad maximum with a peak frequency at luminosities of 6x10^35^ergs/s. 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