Session 111 Interstellar Medium II

Poster, Thursday, January 8, 2004, 9:20am-4:00pm, Grand Hall

111.01 HI Density Distribution Driven by Supernova Ejecta: A Simulation Study

J. A. Hodge (Cal Poly, SLO), A. A. Deshpande (Arecibo Observatory/NAIC, RRI)

111.02 Magnetohydrodynamic Simulations of Shock-Cloud Interactions

K. Gustafson (UM-C), P.C. Fragile, P. Anninos, S.D. Murray (LLNL)

111.03 WHAM Observations of Ionized Gas in High-Velocity Interstellar Clouds

J. L. Reynolds, S. L. Tufte (Lewis & Clark College)

111.04 Evidence for Halo Contributions to the 1/4 keV Diffuse Soft X-Ray Background

E. C. Bellm (Harvard College)

111.05 The Diffuse Ionized Gas as an Indicator for the Galactic Chemical Evolution

T. Elwert, R.-J. Dettmar, R. Teullmann (Astronomisches Institut Ruhr-Universität Bochum, Germany)

111.06 Chlorine in the Galactic Interstellar Medium with FUSE

P. Sonnentrucker (JHU), D. G. York, D. E. Welty (Chicago Univ.), S. D. Friedman (STScI)

111.07 An Enhanced Cosmic-Ray Flux toward \zeta Persei, Inferred from Observations of H₃⁺

B. J. McCall (UC Berkeley), T. R. Geballe (Gemini), T. Oka (U. Chicago)

111.08 A Study of HVCs

E.G. Schmidt, C. Pantoja, M. Lebron (NAIC Arecibo Observatory)

111.09 The Spectroscopy of Plasma Evolution from Astrophysical Radiation (SPEAR) Mission: Early Status and Results

J. Edelstein, E. Korpela (SSL, U.C. Berkeley), K.W. Min, D.H. Lee (SaTReC, KAIST), W.Y. Han, U.W. Nam (KAO), Space Astrophysics Group SPEAR Team, Korea Astronomical Observatory FIMS Team, Satellite Technology Research Center FIMS Team

111.10 Cosmic Rays and Interstellar Turbulence

A. Lazarian, H. Yan (U. Wisconsin)

111.11 Non-isothermal Turbulence in Molecular Clouds

S. C. O. Glover, M.-M. Mac Low (American Museum of Natural History), M. D. Smith, G. Pavlovski, A. Rosen (Armagh Observatory, Northern Ireland)

111.12 A Map of OMC-1 in CO J=9-8 (1.037 THz)

D. P. Marrone, J. Battat, F. Bensch, R. Blundell, T. Hunter, D. Loudkov, S. Paine, C.-Y. E. Tong (CfA), D. Meledin (Chalmers University of Technology), H. Gibson (RPG Radiometer Physics GmbH), S. Radford (NRAO), M. Diaz (Boston University)