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dc.contributor.authorKreimeyer, Kory
dc.contributor.authorBergot, Deanna
dc.contributor.authorLeifeld, Julie
dc.contributor.authorMirocha, Jordan
dc.date.accessioned2010-04-19T18:55:56Z
dc.date.available2010-04-19T18:55:56Z
dc.date.issued2010-04-19T18:55:56Z
dc.identifier.urihttp://hdl.handle.net/2092/1281
dc.descriptionAdvisor: Charles Nelsonen_US
dc.description.abstractSeyfert galaxies are active galaxies characterized by luminous outflows from a central super massive black hole. The outflow mechanism has not been fully determined, but the two primary competing systems are a wind-driven conical outflow and a jet-driven cylindrical outflow. We are developing models with a variety of parameters, including inclination, cone opening angle, etc. By varying these parameters, we can add detail to the model to more completely match the observed velocities. We compare the models to the Hubble Space Telescope long-slit spectra of the Seyfert galaxies NGC 1068 and NGC 4151 in an effort to more fully understand the actual outflow mechanism of these galaxies.en_US
dc.description.sponsorshipDrake University, Department of Physics and Astronomyen_US
dc.language.isoen_USen_US
dc.relation.ispartofseriesDUCURS 2010;32
dc.subjectSeyfert galaxiesen_US
dc.subjectBipolar out-flows (Astrophysics)en_US
dc.subjectHubble Space Telescope (Spacecraft)en_US
dc.titlePowerful Outflows in Seyfert Galaxies : Wind- Vs. Jet-Driven Modelsen_US
dc.typePresentationen_US


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  • DUCURS [196]
    Poster sessions and presentation from the Drake University Conference on Undergraduate Research in the Sciences held each April at Olmsted Center on the Drake campus.

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