Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244...27p&link_type=abstract
Astrophysical Journal, Vol.244, P. 27, 1981
Astronomy and Astrophysics
Astrophysics
5
Scientific paper
The nuclei of two galaxies which show intense [O III] emission lines, NGC 3732, an Sa, and IC 4662, an irregular with a very bright nucleus, are analyzed spectroscopically. The physical condition of the emitting gas and the characteristics and relative degree of evolution of the ionizing sources are discussed.
It was found that the principal differences between the line spectra of both objects are due to abundance effects, although there is some evidence suggesting a different degree of evolution of the ionizing stars.
Dottori Horácio Alberto
Pastoriza Miriani Griselda
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