New Indicators for AGN Power: The Correlation between [O IV] 25.89 μm and Hard X-Ray Luminosity for Nearby Seyfert Galaxies, M. Melendez, S. B. Kraemer, Bryan K. Armentrout, R. P. Deo, D. M. Crenshaw, H. R. Schmitt, R. F. Mushotzky, J. Tueller, C. B. Markwardt, L. Winter
Bryan Armentrout

New Indicators for AGN Power: The Correlation between [O IV] 25.89 μm and Hard X-Ray Luminosity for Nearby Seyfert Galaxies, M. Melendez, S. B. Kraemer, Bryan K. Armentrout, R. P. Deo, D. M. Crenshaw, H. R. Schmitt, R. F. Mushotzky, J. Tueller, C. B. Markwardt, L. Winter
Chemistry and Physics Faculty Articles