Abstract: | The results of a spectroscopic investigation of galaxies Nos. 22, 35, 133, 317, and 321 from the lists of M. A. Kazarian,
Astrofizika,15, 5 (1979); M. A. Kazarian and é. S. Kazarian, Astrofizika,16, 17 (1980)] are given. The equivalent widths of lines, the relative intensities of emission lines, and their half-widths
are determined.
Translated from Astrofizika, Vol. 40, No. 4, pp. 619–626, October-December, 1997. |