Bibcode
Rozas, M.; Beckman, J. E.; Knapen, J. H.
Referencia bibliográfica
Astronomy and Astrophysics, v.307, p.735-744
Fecha de publicación:
3
1996
Revista
Número de citas
90
Número de citas referidas
75
Descripción
We present new high quality continuum-subtracted Hα images of the
grand-design galaxies NGC 157, NGC 3631, NGC 6764 and NGC 6951. We have
determined the positions, angular sizes, and fluxes of their individual
HII regions, and describe statistical properties of the HII region
samples. We construct luminosity functions for all the HII regions in
the disc and separately for arm and interarm zones for each galaxy. The
slopes of the luminosity functions for the complete sample agree well
with values published for other spiral galaxies of comparable
morphological type. For three galaxies we determined the slopes of the
luminosity functions for the spiral arm and interarm zones separately.
We find that for NGC 157, NGC 3631, and NGC 6951 these slopes are equal
within the errors of determination. We compare our results to those
found from earlier work, specifically for M51 and NGC 6814, and discuss
implications for massive star forming processes.