Active Galactic Nuclei


NGC 1566 pictured above is an example of a Seyfert galaxy. It has a bright point, central nucleus whose spectrum shows charactistic broad emission lines. The lines are attributed to gas moving at velocities of thousands of km/s aound a supermassive black hole. The picture was taken on the UK Schmidt Telescope


Much of my work on Active Galactic Nuclei for the past several years has been in collaboration with my former graduate student Alex Filippenko (U.C. Berkeley and his former students (and, therefore, my grandchildren) L. Ho (OCIW) and A. Barth (CfA). Our major work was a survey of the nuclei of the brightest 500 galaxies north of the celestial equator using sectra obtained with the Double Spectrograph on the Hale 200 inch telescope at the Palomar Observatory . This survey, which was started when Filippenko was my student in 1984 and completed in 1998, took about 50 clear nights and could only have been done by people with priviledged access to a large telescope. Click here to see a figure from the paper by Ho, Filippenko, Peng and Sargent referred to below. It shows typical examples of how the H alpha and [N II] lines were decomposed into broad and sharp components in order to reveal the broad H alpha emission line characteristic of a Seyfert I galaxy.


Some of our papers are listed below:


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page by Wallace Sargent, last updated 19 May 1999