Spectroscopy of two ultraviolet-excess galaxies

Details Spectroscopy of two ultraviolet-excess galaxies Spectroscopy of two ultraviolet-excess galaxies

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..276k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 7, May 1981, p. 276-279.) Soviet Astronomy Letters, vol. 7, May-June 1981, p. 153, 154.

Astronomy and Astrophysics

Astronomy

5

Astronomical Spectroscopy, Galaxies, Ultraviolet Astronomy, Ultraviolet Spectra, Astronomical Photography, Emission Spectra, Line Spectra

Scientific paper

Results are presented from spectroscopic observations of galaxies Nos. 138 and 212, which have ultraviolet excesses and are listed by Kazaryan (1980). Both galaxies exhibit H I, and forbidden S II, O III, and O II emission lines. Both have Balmer decrement from gaseous nebulas, and galaxy No. 212 contains three superassociations, which indicates vigorous star formation. Equivalent widths along with relative intensities are determined for the emission lines observed in the two galaxies.

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