UV and optical observations of PG 1351+64 - A bright Seyfert galaxy or a low-luminosity QSO

Details UV and optical observations of PG 1351+64 - A bright Seyfert galaxy or a low-luminosity QSO UV and optical observations of PG 1351+64 - A bright Seyfert galaxy or a low-luminosity QSO

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.216..529t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 216, Oct. 1, 1985, p. 529-536.

Astronomy and Astrophysics

Astronomy

9

Quasars, Seyfert Galaxies, Spectral Energy Distribution, Ultraviolet Spectra, Continuous Spectra, Iue, Line Spectra, Spectrophotometry, Variability

Scientific paper

PG 1351+64 was repeatedly observed in 1979 - 83 with IUE. Variations of a factor of 2 in both line and continuum intensity were observed with a time-scale of ≡1 month. Coordinated optical observations suggest that the ultraviolet variability is not accompanied by optical variability, so that the overall energy distribution changes shape. The properties of the object are compared with those of Seyfert I galaxies and QSOs.

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