Session 51. Radio Galaxies

Display, Tuesday, January 8, 2002, 9:20am-6:30pm, Exhibit Hall

51.01 Are Quasars Ejected from the Nucleus of NGC 4258?

P. T. Kondratko, L. J. Greenhill, J. M. Moran (CfA)

51.02 STIS spectroscopy of gas disks in the nuclei of nearby, radio-loud elliptical galaxies.

J. Noel-Storr (Columbia University), S. A. Baum (STScI), C. M. Carollo (Columbia University), C. P. O'Dea (STScI), G. A. Verdoes Kleijn (Leiden University), R. P. van der Marel (STScI), P. T. de Zeeuw (Leiden University)

51.03 Preliminary Results from an XMM-Newton Observation of the Nearby Radio Galaxy Centaurus A

S. Vazquez (U Puerto Rico/Harvard-Smithsonian CfA), R.P. Kraft, W.R. Forman, C. Jones, S.S. Murray (Harvard-Smithsonian CfA), M.J. Hardcastle, D.M. Worrall (University of Bristol)

51.04 Orientation of Jets Relative to Dust Disks in Radio Galaxies

H. R. Schmitt (NRAO - Socorro), J. E. Pringle, C. J. Clarke (Institute of Astronomy - Cambridge), A. L. Kinney (NASA)

51.05 Ultraviolet Images of Nearby Radio Galaxies

W.B. Sparks, M.G. Allen, C.P. O'Dea, A. Koekemoer (STScI), A.R. Martel (Johns Hopkins University)

51.06 The Nature of Radio-optical Alignments in Faint Radio Sources

S.E. Ridgway (JHU), M.D. Lacy (IGPP,LLNL)

51.07 Shapes of Synchrotron Spectra from Fanaroff-Riley II sources

E. Grundstrom, L. Rudnick (University of Minnesota), K. M. Blundell (University of Oxford)

51.08 Emission Line Diagnostics of Accretion Flows in Weak-Line Radio Galaxies

K. T. Lewis, M. Eracleous, R. M. Sambruna (Penn. State U.)

51.09 Spectral Shapes of Relaxed Radio Galaxy Lobes

A. Young, L. Rudnick (U. Minnesota), K. Makishima, M. Tashiro, N. Iyomoto (U. Tokyo), N. Kassim (NRL), D. Worrall (Bristol)

51.10 Multi-Scale Structures in Chandra Images of Cen A

M. Karovska, G. Fabbiano, M. Elvis, S.S. Murray, R. Kraft, F. Nicastro, M. Juda, T. Aldcroft, T. Gaetz, D. Jerius, A. Kenter (Harvard-Smithsonian CfA)

51.11 Chandra observations of the nearby low-power radio galaxy NGC 4261

A. Rinn, R.M. Sambruna (GMU)

51.12 Exploring magnetic fields around supermassive black holes using Faraday Rotation.

R.T. Zavala (National Radio Astronomy Observatory, New Mexico State University), G.B. Taylor (National Radio Astronomy Observatory)