The profile of emission lines formed during the motion of clouds in jets in active galactic nuclei

Details The profile of emission lines formed during the motion of clouds in jets in active galactic nuclei The profile of emission lines formed during the motion of clouds in jets in active galactic nuclei

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67..463z&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, May-June 1990, p. 463-471. In Russian.

Astronomy and Astrophysics

Astronomy

1

Active Galactic Nuclei, Emission Spectra, Molecular Clouds, Seyfert Galaxies, Equations Of Motion, H Beta Line, Satellite Observation

Scientific paper

Formulas are derived describing the profile of emission lines formed during the motion of emission clouds inside a conical jet with a small opening angle. It is assumed that the clouds are accelerated by radiation of the central body. Based on the width of the satellites observed at both sides of the H-beta line in the spectrum of the Seyfert galaxy NGC 4151, a jet opening angle of about 5 deg is estimated for this object.

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