Spectral and morphological study of galaxies with UV excess. VI

Details Spectral and morphological study of galaxies with UV excess. VI Spectral and morphological study of galaxies with UV excess. VI

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..431k&link_type=abstract

(Astrofizika, vol. 22, May-June 1985, p. 431-440) Astrophysics (ISSN 0571-7132), vol. 22, no. 3, Nov. 1985, p. 253-259. Translat

Astronomy and Astrophysics

Astrophysics

6

Galactic Structure, Gas Composition, Mass Distribution, Spectrum Analysis, Ultraviolet Spectra, Astronomical Spectroscopy, Emission Spectra, Line Shape, Spectral Line Width

Scientific paper

The results of spectrophotometry and morphology of galaxies No. 73, 125 and 229 from the lists (1979) are presented. The masses of the gaseous component of these galaxies are obtained. It has been established that galaxy No. 73 is of Sy 2 type and by its physical properties is similar to the Sy 2 type galaxies Mark 744 and 1066. Though the galaxy No. 125 by its several properties is similar to No. 73, it is, however, evidently in a later stage of evolution than galaxy No. 73.

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