Accretion disk in the high-redshift quasar HS 1700+6416.
Bibcode: 1990A&A...231L...1S
Siemiginowska, A.; Dobrzycki, A.
Poland
Abstract
We apply the standard accretion disk model to reproduce the EUV spectrum of the high-redshift (z = 2.72) quasar HS 1700+6416. We find a satisfactory fit to the observed spectrum. The contribution of the accretion disk to the continuum emission in the soft X-ray spectral region may be significant.
1990
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Astronomy and Astrophysics
IUE
5