A detailed study of the CIV 1550 line profile and adjacent spectral features in NGC4151 from 1978 up to 1983

Astronomy and Astrophysics – Astrophysics

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Galactic Radiation, Line Spectra, Seyfert Galaxies, Accretion Disks, Periodic Variations, Spectral Line Width, Ultraviolet Spectra

Scientific paper

The 1450 to 1720 A interval in the UV spectrum of the Seyfert 1 galaxy NGC 4151 was examined, using line profile fitting techniques to study temporal variations at 69 different epochs from 1978 to 1983. Over a distance range from 5 light-days up to 500 light-years from the nucleus, the velocity law is Keplerian. An intermediate region, whose density (10 million cc) velocity dispersion (1600 km/sec) and dimension (250 light-days) are intermediate between those of the broad and narrow line regions is identified. Evidence of gas expanding at 4000 km/sec at a few light-days from the nucleus is found. This outflow is presumably decelerated outward and partially obscured by an accretion disk seen almost edge-on.

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