UV and optical variability of the low luminosity quasar PG 1351+64

Details UV and optical variability of the low luminosity quasar PG 1351+64 UV and optical variability of the low luminosity quasar PG 1351+64

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..617t&link_type=abstract

In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 617-61

Astronomy and Astrophysics

Astrophysics

2

Quasars, Stellar Spectra, Ultraviolet Spectra, Variability, Iue, Line Spectra, Lyman Alpha Radiation

Scientific paper

PG 1351+64 is a bright radio quiet quasar (z = 0.088, mV ≅ 14). IUE observations obtained within few months in 1982 - 1983 showed variations in the 1200 - 2000 Å band up to a factor of 2. Since then the object has been monitored regularly. The observations of 1984 - 1986, including also archival data, have more than doubled the number of available spectra in the UV. In particular the source was found in its brightest state, both in the optical and UV bands, in 1986 February.

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