Mass outflow constraints in active nuclei and quasars from X-ray spectroscopy

Details Mass outflow constraints in active nuclei and quasars from X-ray spectroscopy Mass outflow constraints in active nuclei and quasars from X-ray spectroscopy

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..245..263y&link_type=abstract

Formation and Evolution of Galaxy Bulges, Proceedings of the International Astronomical Union, IAU Symposium, Volume 245, p. 263

Astronomy and Astrophysics

Astronomy

Galaxies: Active, Ism: Jets And Outflows, X-Rays: Galaxies

Scientific paper

Absorption in the X-ray spectra of active galactic nuclei from outflowing gas can be modeled to yield critical physical information on the outflows. The outflow rate of mass ejected back into the ISM of the host galaxy and the resulting feedback could potentially have an impact on evolution. We give a brief overview of the current observational constraints on the outflows that should be taken into account by models of evolution and feedback.

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