Non-relativistic outflows in active galactic nuclei

Details Non-relativistic outflows in active galactic nuclei Non-relativistic outflows in active galactic nuclei

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pabei..19..232w&link_type=abstract

Progress in Astronomy, Vol. 19, No. 2, p. 232 - 236 (2001). In: Proceedings for the First National Academic Conference of the Ch

Astronomy and Astrophysics

Astronomy

Quasars, Absorption Lines, Seyfert Galaxies, X Rays, Ultraviolet

Scientific paper

Two type outflows are seen in active galactic nuclei (AGN). Characterizing by their non-thermal radiation, relativistic radio jets are detected mainly in radio loud AGN, while non-relativistic outflow is observed through blue-shifted absorption lines in both radio loud and radio quiet AGN. Some new results on the mass outflow in the quasars and Seyfert galaxies from UV and X-ray observations are summarized. These results highlight the importance of mass loss process in broad absorption line quasars.

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