UV spectrum of quasar 0916+558

Details UV spectrum of quasar 0916+558 UV spectrum of quasar 0916+558

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.281c&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 281-282 (SEE N89

Astronomy and Astrophysics

Astronomy

Cerenkov Radiation, Iue, Quasars, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Spectra, Astronomical Models, Emission Spectra, Lyman Spectra, Red Shift, Spectral Energy Distribution

Scientific paper

The UV spectrum of QSO 0916+558 was observed IUE. The intensity ratios of emission lines of QSO 0916+558 were compared with theoretical models, suggesting that Cerenkov line emission mechanism may play an important role. Combining the observed continua, fluxes, and equivalent widths of Lyman alpha and C IV emission lines with UV data for other quasars, the Baldwin effect is also discussed.

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