Spectrophotometric investigation of a quasistellar object

Details Spectrophotometric investigation of a quasistellar object Spectrophotometric investigation of a quasistellar object

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981afz....17..661k&link_type=abstract

(Astrofizika, vol. 17, Oct.-Dec. 1981, p. 661-666.) Astrophysics, vol. 17, no. 4, Apr. 1982, p. 354-357. Translation.

Astronomy and Astrophysics

Astrophysics

7

Balmer Series, Emission Spectra, Galactic Nuclei, Quasars, Seyfert Galaxies, Spectral Line Width, Spectrophotometry, Forbidden Bands, H Lines, Luminosity, Ubv Spectra

Scientific paper

A spectrophotometric investigation of quasi-stellar object 102 in the catalog of galaxies with UV excess has yielded profiles whose emission line equivalent widths and relative intensities are presented. Object 102 displays a luminosity which is situated between that of Seyfert galaxies and quasars, leading to the conclusion that quasi-stellar objects and Seyfert 1 galaxies may be considered as members of a new class on the basis of their physical characteristics.

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