Simulations of Stellar Feedback in Nearby AGN

Details Simulations of Stellar Feedback in Nearby AGN Simulations of Stellar Feedback in Nearby AGN

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sacm.confe..22s&link_type=abstract

The Starburst-AGN Connection under the Multiwavelength Limelight, held 14-16 September 2011. Published online at http://www.scio

Computer Science

Scientific paper

I will report on our effort to simulate the connection between stellar mass loss and energy feedback from nuclear star clusters and bulges of nearby Seyfert galaxies. We use observations of stellar kinematics and density to constrain high-resolution hydrodynamical simulations and compare the resulting density distributions to available high resolution simulations. We investigate under which conditions such stellar feedback might lead to the formation of a nuclear gas disk or torus and to nuclear activity cycles.

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