Dynamics of the radiating gas in the quasar PHL 5200 and in kindred objects

Details Dynamics of the radiating gas in the quasar PHL 5200 and in kindred objects Dynamics of the radiating gas in the quasar PHL 5200 and in kindred objects

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59.1070g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Nov.-Dec. 1982, p. 1070-1074) Soviet Astronomy (ISSN 0038-5301), vol. 26, Nov.-Dec. 1982, p.

Astronomy and Astrophysics

Astronomy

1

Galactic Nuclei, Plasma Radiation, Quasars, Seyfert Galaxies, Emission Spectra, Gas Flow, Kinematics, Line Spectra, Resonance Lines, Spectrum Analysis, Velocity Distribution

Scientific paper

Recent interpretations of the peculiar resonance-line profiles in the spectrum of PHL 5200 have suggested that a radially symmetric, outward decelerating flow is issuing from the nucleus of this quasar. The braking mechanism is briefly discussed, and an explanation is offered for the unique emission spectrum. Qualitatively, however, the kinematic conditions in th PHL 5200 envelope resemble the velocity field in other quasar and Seyfert-nucleus envelopes.

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