Accretion disk in the high-redshift quasar HS 1700+6416.
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.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- May 1990
- Bibcode:
- 1990A&A...231L...1S
- Keywords:
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- Accretion Disks;
- Extreme Ultraviolet Radiation;
- Quasars;
- Red Shift;
- Astronomical Models;
- Black Holes (Astronomy);
- Iue;
- Astrophysics