Interpretation of the spectrum of the QSO 1303 + 308

Details Interpretation of the spectrum of the QSO 1303 + 308 Interpretation of the spectrum of the QSO 1303 + 308

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..782v&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Sept. 1990, p. 782-784. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Plasma Dynamics, Quasars, Spectrum Analysis, Cosmic Plasma, Resonance Lines

Scientific paper

A mathematical continuous outflow model based on the theory of plasma dynamics in a radiation field is used to interpret spectra from the QSO 1303 + 308. Radiation transfer in spectral lines is examined using the Sobolev (1947) approximation. The spectra of QSO 1303 + 308 are calculated for the blue wings of resonance lines for the ions C IV, N V, and Si IV. Graphs are provided of intensity plotted against flow velocity.

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