Metal Rich H 11 Regions: the Size of the Ionizing Cluster

Details Metal Rich H 11 Regions: the Size of the Ionizing Cluster Metal Rich H 11 Regions: the Size of the Ionizing Cluster

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993rmxaa..27..195t&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 27, 195

Astronomy and Astrophysics

Astronomy

Scientific paper

RESUMEN Los cumulos ionizantes en regiones HIl de alta metalicidad parecen ser ma's pequefios que aque'llos en regiones de baja metalicidad. Proponemos aqui una posible explicaci6rf para este fen6meno. ABSTRACT The sizes of the ionizing clusters in metal-rich HIl regions seem to be smaller than their low metallicity counterparts. The possible origin for this behavior is discussed. Key words: GALAXIES: ISM GALAXIES: STELLAR CONTENT H II REGIONS

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