Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218...65n&link_type=abstract
In ESA Fourth European IUE Conf. p 65-68 (SEE N84-35135 24-88)
Astronomy and Astrophysics
Astronomy
Galactic Nuclei, Iue, Ultraviolet Astronomy, Ultraviolet Spectra, Cosmic Dust, H Ii Regions, Interstellar Matter, Luminous Intensity, Markarian Galaxies, O Stars
Scientific paper
The UV flux distributions of several hot spot galaxies were obtained with the IUE in the low dispersion, large aperture mode. The UV spectra do not suggest the presence of O type stars in marked contrast to Markarian galaxies. The NIII lambda, 1750 and CIII lambda 1909 lines from high excitation HII regions or planetary nebulae are not present. The UV flux distributions were used to determine the population of early type stars. They show evidence of reddening but the lambda 2200 dust feature is clearly absent.
Nandy K.
Thompson G. I.
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