Line Forming Regions in Active Galaxies and their Nuclei

Details Line Forming Regions in Active Galaxies and their Nuclei Line Forming Regions in Active Galaxies and their Nuclei

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.237..187d&link_type=abstract

Astrophysics and Space Science, Volume 237, Issue 1-2, pp. 187-206

Astronomy and Astrophysics

Astrophysics

Scientific paper

The spectra of active galaxies and their nuclei are rich in emission and absorption line features. A major aim of present research is the development of self-consistent hydrodynamic models for the production of the line-forming regions. We here review such modelling and stress the central role played by shock phenomena induced by winds and explosions on scales ranging from the circumstellar to the intergalactic.

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