UV observations on the variable quasar PG 1351+64

Details UV observations on the variable quasar PG 1351+64 UV observations on the variable quasar PG 1351+64

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..119t&link_type=abstract

In ESA Fourth European IUE Conf. p 119-124 (SEE N84-35135 24-88)

Physics

1

Quasars, Ultraviolet Spectra, Variable Stars, Continuous Radiation, Iue, Spectral Energy Distribution, Stellar Mass

Scientific paper

The bright low red shift quasi stellar object PG 1351+64 was repeatedly observed with IUE. The spectra exhibit strong emission lines superposed to a continuum with a spectral index of -0.3 for a single power low fit in the 1200 to 3000 A range. Variations of a factor 2 in line and continuum intensity are observed with a minimum time scale of a month. The nature of the continuum emission is discussed and an upper limit to the mass within the line emitting region is deduced from the observed line variability.

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