Accretion disk in the high-redshift quasar HS 1700 + 6416

Details Accretion disk in the high-redshift quasar HS 1700 + 6416 Accretion disk in the high-redshift quasar HS 1700 + 6416

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231l...1s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 1, May 1990, p. L1, L2.

Astronomy and Astrophysics

Astronomy

5

Accretion Disks, Extreme Ultraviolet Radiation, Quasars, Red Shift, Astronomical Models, Black Holes (Astronomy), Iue

Scientific paper

The standard accretion disk model is applied to reproduce the EUV
spectrum of the high-redshift (z = 2.72) quasar HS1700 + 6416. A
satisfactory fit to the observed spectrum is found. The contribution of
the accretion disk to the continuum emission in the soft X-ray spectral
region may be significant.

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