Far ultraviolet observations of the quasar PG1351+64

Details Far ultraviolet observations of the quasar PG1351+64 Far ultraviolet observations of the quasar PG1351+64

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..299m&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

4

Iue, Quasars, Ultraviolet Astronomy, Absorption Spectra, Carbon, Continuous Spectra, Emission Spectra, Lyman Alpha Radiation, Magnesium, Nitrogen, X Ray Sources

Scientific paper

Short and long wavelength spectra of the low red-shift QSO PG1351+64, obtained with International Ultraviolet Explorer, are presented. The continuum can be fitted by a power law F lambda varies as lambda to the 0.2 power, with a luminosity of 9 x 10 to the 44th power ergs/sec between 1200 and 3200 A. The eq.w. of lyman alpha is 100 A with a FWHM of 12 A. Strong local absorption is observed in the C IV line (+1780 km/sec). The results are discussed with respect to the suggested correlations between quasar properties.

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