The correlation between morphological type and the diameters of the largest HII complexes in galaxies is interpreted theoretically as a consequence of the rate of stellar formation of massive stars and the original luminosity function in galaxies.
General information
Issue date:1963
Document language:English
Journal:Boletín de la Asociación Argentina de Astronomía; no. 6
Event:VI Reunión Científica de la Asociación Argentina de Astronomía (Horco Molle, Tucumán, 22 al 25 de mayo de 1963)
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