Proceedings of "The Riddle of Cooling Flows in Galaxies and Clusters of Galaxies"

The proceedings are published electronically through this conference web site. The long time availability is made certain by inclusion of the full text into the ADS (after three years according to ADS policy).

Bibliographic information for the proceedings is as follows:
Title: The Riddle of Cooling Flows in Galaxies and Clusters of Galaxies
Location and date: Charlottesville, VA, USA. May 31 – June 4, 2003.
URL: http://www.astro.virginia.edu/coolflow/
Editors: Reiprich, T. H., Kempner, J. C., and Soker, N.
BibTeX entry: from ADS

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US   The entire proceedings may be downloaded in a single volume using the icons to the left. Some of the figures in the PDF versions may not display properly due to errors in the original files. The figures in the postscript versions do not have this problem. The PDF problems occur in both the single volume and the individual articles. The postscript files are about 36 MB each (173 MB uncompressed); the PDF files are about 24 MB each.
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Table of Contents

  1. Poster Session
  2. Observations: Cooling Rate
  3. Observations: Cool Gaseous Material and Intrinsic Absorption
  4. Observations: Magnetic Fields
  5. Observations: Radio Properties and Star Formation in Cooling Cores
  6. Observations: Interaction Radio/X-Ray Plasma
  7. Observations: Temperature, Gas/Dark Matter Density, and Chemical Abundance Structure
  8. Observations: Cooling in Normal Ellipticals
  9. Questions: Do Cooling Flows Exist and if so How Much Gas Cools to How Low Temperatures?
  10. Questions: What is the Fate of the Cooling Gas?
  11. Questions: What is the Mutual Interaction of AGN and X-Ray Gas?
  12. Questions: What (Other) Heating Mechanisms Affect Cooling Gas?
  13. Questions: What is the Role of Magnetic Fields in Cooling Flows?
  14. Questions: What is the Chemical and Temperature Structure of the Central Gas?
  15. Questions: What are the Effects of Cluster Dynamics on Cooling Flows?
  16. Questions: How Do Cluster Cores Evolve Cosmologically and Affect the Use of Clusters as Cosmological Probes?
  17. Meeting Summary
  18. Conference Notes

1. Poster Session

US   Constraining Multiphase Gas in Cooling Flows
Arabadjis, J. S. (MIT); Bautz, M. W. (MIT)
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US   Polarized Emission Throughout the Perseus Cluster
Brentjens, M. A. (Kapteyn Institute, Groningen ASTRON, Dwingeloo); de Bruyn, A. G. (ASTRON, Dwingeloo Kapteyn Institute, Groningen)
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US   Heating, Cooling and Conduction in Galaxy Clusters
Brüggen, M. (International University Bremen)
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US   Radio and X-Ray Interactions in the Core of Abell 2029
Clarke, T.E. (University of Virginia); Blanton, E.L. (University of Virginia); Sarazin, C.L. (University of Virginia)
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US   XMM-Newton Observation of the Cooling-Flow Cluster Abell 478
de Plaa, J. (SRON National Institute for Space Research, Utrecht, The Netherlands); Kaastra, J. S. (SRON National Institute for Space Research, Utrecht, The Netherlands); Tamura, T. (ISAS Institute of Space and Astronautical Science, Kanagawa, Japan); Mendez, M. (SRON National Institute for Space Research, Utrecht, The Netherlands); Peterson, J. R. (Astrophysics Laboratory, Columbia University, New York, USA); Pointecouteau, E. (CEA/DSM/DAPNIA Saclay, Service d’Astrophysique, Gif-sur-Yvette, France); Arnaud, M. (CEA/DSM/DAPNIA Saclay, Service d’Astrophysique, Gif-sur-Yvette, France)
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US   Next Generation of Galaxy Cluster Simulations
Dolag, K. (Dipartimento di Astronomia, Università di Padova, Italy)
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US   Mapping the Molecular Hydrogen Emission in the Cooling Flow Cluster Abell 1795
Edwards, L. O. V. (Saint Mary’s University)
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US   Cooling Flows and Radio Mini-Halos in Clusters of Galaxies
Gitti, M. (Institute of Astrophysics, University of Innsbruck – Dipartimento di Astronomia, Università di Bologna – Istituto di Radioastronomia del CNR, Bologna); Brunetti, G. (Istituto di Radioastronomia del CNR, Bologna); Setti, G. (Dipartimento di Astronomia, Università di Bologna – Istituto di Radioastronomia del CNR, Bologna); Feretti, L. (Istituto di Radioastronomia del CNR, Bologna)
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US   Brightness Discontinuities in the Northern Sub-Cluster of Abell 115
Gutierrez, K. (Washington University in St. Louis); Krawczynski, H. (Washington University in St. Louis); Harris, D. (Smithsonian Astrophysical Observatory)
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US   Non-Thermal Emission From IC1262, a Low Temperature Galaxy Cluster
Hudson, D. S. (Joint Center for Astrophysics, University of Maryland Baltimore); Henriksen, M. J. (Joint Center for Astrophysics, University of Maryland Baltimore); Colafrancesco, S. (Osservatorio Astronomico di Roma)
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US   The Magnetic Field in A3667
Johnston-Hollitt, M. (Leiden Observatory)
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US   Chandra Observation of the Core of Abell 576
Kempner, J. C. (Harvard-Smithsonian Center for Astrophysics); David, L. P. (Harvard-Smithsonian Center for Astrophysics)
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US   Observations of Central Radio Sources in Cooling Core Clusters
Markovi’c, T. (NRAO, New Mexico Tech); Owen, F.N. (NRAO); Eilek, J.A. (New Mexico Tech)
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US   The Impact of Star Formation On Cool Core Galaxy Clusters
Motl, P. M. (University of Colorado, Center for Astrophysics and Space Astronomy); Burns, J. O. (University of Colorado, Center for Astrophysics and Space Astronomy); Normal, M. L. (University of California, San Diego, Center for Astrophysics and Space Sciences); Bryan, G. L. (University of Oxford)
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US   AWM 4 and MKW 4 - Two Very Different Poor Clusters Observed with XMM-Newton
O’Sullivan, E. (Harvard-Smithsonian Center for Astrophysics); Vrtilek, J. M. (Harvard-Smithsonian Center for Astrophysics)
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US   The Spontaneous Magnetic Field Generation and Suppression of Heat Conduction in Clusters of Galaxies
Okabe, N. (Astronomical Institute, Tohoku University); Hattori, M. (Astronomical Institute, Tohoku University)
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US   SMAUG: A New Technique for the Deprojection of Galaxy Clusters
Pizzolato, F. (Istituto di Fisica Cosmica, IASF/CNR, MILANO -Italy)
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US   Simulations of Rising Hydrodynamic and Magnetohydrodynamic Bubbles
Ricker, P. M. (Dept. of Astronomy, University of Illinois at Urbana-Champaign and National Center for Supercomputing Applications); Robinson, K. (ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Dursi, L. J. (Dept. of Astronomy and Astrophysics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Rosner, R. (Dept. of Physics, Dept. of Astronomy and Astrophysics, and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Calder, A. C. (Dept. of Astronomy and Astrophysics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Zingale, M. (Dept. of Astronomy and Astrophysics, University of California at Santa Cruz); Truran, J. W. (Dept. of Astronomy and Astrophysics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Linde, T. (Dept. of Astronomy and Astrophysics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Caceres, A. (Dept. of Physics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Fryxell, B. (Dept. of Astronomy and Astrophysics and ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Olson, K. (UMBC/GEST Center, NASA Goddard Space Flight Center); Riley, K. (ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Siegel, A. (ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago); Vladimirova, N. (ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago)
US

US   Chandra Observations of the Central Region of Abell 3112
Takizawa, M. (Yamagata University); Sarazin, C. L. (University of Virginia); Blanton, E. L. (University of Virginia); Taylor, G. B. (National Radio Astronomy Observatory)
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US   The Turmoil in IC1262
Trinchieri, G. (INAF-OAB); Saporiti, C. (Università degli Studi - Milano)
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US   Simulations of Cooling Flow Clusters with Thermal Conduction
Ziskin, V. (Institut d’Astrophysique de Paris)
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2. Observations: Cooling Rate

US   High Resolution X-Ray Spectroscopic Constraints On Cooling-Flow Models
Peterson, J. R. (Columbia University); Kahn, S. M. (Columbia University); Paerels, F. B. S. (Columbia University); Kaastra, J. S. (SRON); Tamura, T. (SRON); Bleeker, J. A. M. (SRON); Ferrigno, C. (SRON); Jernigan, J. G. (UC Berkeley)
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US   The ASCA View On Cooling Flows and Its Implications
Makishima, K. (Department of Physics, University of Tokyo)
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US   XMM-Newton Observation of the Centaurus Cluster
Takahashi, I. (University of Tokyo); Kawaharada, M. (University of Tokyo); Makishima, K. (University of Tokyo); Ikebe, Y. (JCA UMBC GSFC); Tamura, T. (SRON ISAS)
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3. Observations: Cool Gaseous Material and Intrinsic Absorption

US   Cold Molecular Gas in Abell 1795
Salomé, P. (LERMA, Observatoire de Paris); Combes, F. (LERMA, Observatoire de Paris)
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4. Observations: Magnetic Fields

US   Magnetic Fields and Cosmic Rays in Galaxy Cluster Cooling Flows
Enßlin, T. A. (Max-Planck-Institut für Astrophysik); Vogt, C. (Max-Planck-Institut für Astrophysik); Pfrommer, C. (Max-Planck-Institut für Astrophysik)
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US   A Critical Look at Faraday Rotation Measures of Cluster Magnetic Fields
Rudnick, L. (University of Minnesota); Blundell, K. M. (Oxford University)
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5. Observations: Radio Properties and Star Formation in Cooling Cores

US   The Low Frequency Array and Clusters of Galaxies
Kassim, N. (Naval Research Laboratory); Cohen, A. (Naval Research Laboratory and National Research Council); Lazio, T. J. W. (Naval Research Laboratory)
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US   Radio Galaxies in Cooling Cores
Eilek, J. A. (New Mexico Tech)
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US   Star Formation in Cluster Cooling Flows
McNamara, B. R. (Ohio University)
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6. Observations: Interaction Radio/X-Ray Plasma

US   The Interaction of Radio Sources and X-Ray-Emitting Gas in Cooling Flows
Blanton, E. L. (University of Virginia, Chandra Fellow)
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US   Self Regulated AGN Interaction with Cluster Cooling Core Regions: The Metallicity Distribution As Diagnostic
Boehringer, H. (Max-Planck-Institut fuer extraterr. Physik); Matsushita, K. (Tokyo University of Science); Churazov, E. (Max-Planck-Institut fuer Astrophysik); Finoguenov, A. (Max-Planck-Institut fuer extraterr. Physik)
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7. Observations: Temperature, Gas/Dark Matter Density, and Chemical Abundance Structure

US   X-Ray Measurement of Dark Matter
Ikebe, Y. (Joint Center for Astrophysics, University of Maryland); Boehringer, H. (Max-Planck-Institut fuer extraterrestrische Physik); Kitayama, T. (Department of Physics, Toho University)
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US   Ni Abundance in the Core of the Perseus Cluster: An Answer To the Significance of Resonant Scattering
Gastaldello, F. (IASF - CNR); Molendi, S. (IASF - CNR)
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8. Observations: Cooling in Normal Ellipticals

US   Elliptical Galaxy Cooling Flows
Bregman, J. N. (University of Michigan); Athey, A. E. (University of Michigan)
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US   Can Mergers Explain Cooling Flows?
Sparks, W. B. (Space Telescope Science Institute); Donahue, M. (Michigan State University)
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9. Questions: Do Cooling Flows Exist and if so How Much Gas Cools to How Low Temperatures?

US   Cooling Flows Or Heating Flows?
Binney, J. (Oxford University)
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10. Questions: What is the Fate of the Cooling Gas?

US   What Is the Fate of the Cooling Gas?
Voit, G. M. (Michigan State University)
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US   Entropy Evolution of the Gas in Cooling Flow Clusters
Kaiser, C. R. (University of Southampton); Binney, J. J. (University of Oxford)
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11. Questions: What is the Mutual Interaction of AGN and X-Ray Gas?

US   The Interaction of Jets with the Intracluster Medium
Heinz, S. (Max-Planck-Institute for Astrophysics, Garching, Germany); Enßlin, T. (Max-Planck-Institute for Astrophysics, Garching, Germany)
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US   Interaction of the AGN and X-Ray Emitting Gas
Nulsen, P. (University of Wollongong and Harvard-Smithsonian Center for Astrophysics)
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12. Questions: What (Other) Heating Mechanisms Affect Cooling Gas?

US   Heating of Cluster Cores By Acoustic Waves
Fujita, Y. (National Astronomical Observatory); Suzuki, T. K. (Department of Physics, Kyoto University)
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13. Questions: What is the Role of Magnetic Fields in Cooling Flows?

US   Cooling of X-Ray Emitting Gas By Heat Conduction in the Center of Cooling Flow Clusters
Soker, N. (Technion-Israel Institute of Technology); Blanton, E. L. (University of Virginia); Sarazin, C. L. (University of Virginia)
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US   Intracluster Magnetic Fields and the Reheating of Cooling Flows
De Young, D. S. (NOAO)
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14. Questions: What is the Chemical and Temperature Structure of the Central Gas?

US   XMM-Newton Observations of the Temperature Structure of the Central Gas in Cooling Clusters
Kaastra, J. S. (SRON National Institute for Space Research, Utrecht, The Netherlands); Tamura, T. (SRON National Institute for Space Research, Utrecht, The Netherlands, and Institute of Space and Astronautical Science (ISAS), Kanagawa, Japan ); Peterson, J. R. (Columbia Astrophysics Laboratory, Columbia University); Bleeker, J. A. M. (SRON National Institute for Space Research, Utrecht, The Netherlands); Ferrigno, C. (SRON National Institute for Space Research, Utrecht, The Netherlands, and Istituto di Astrofisica Spaziale e Fisica Cosmica, Sezione di Palermo, Palermo, Italy); Kahn, S. M. (Columbia Astrophysics Laboratory, Columbia University, and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University); Paerels, F. B. S. (Columbia Astrophysics Laboratory, Columbia University); Piffaretti, R. (Institute of Theoretical Physics, University of Zürich, Zürich, Switzerland, and Paul Scherrer Institute, Laboratory for Astrophysics, Villigen, Switzerland); Branduardi-Raymont, G. (Mullard Space Science Laboratory, University College London, Surrey, UK); Böhringer, H. (Max-Planck-Institut für extraterrestrische Physik, Garching, Germany)
US

15. Questions: What are the Effects of Cluster Dynamics on Cooling Flows?

US   On the Formation of Cool, Non-Flowing Cores in Galaxy Clusters Via Hierarchical Mergers
Burns, J. O. (University of Colorado, Center for Astrophysics and Space Astronomy); Motl, P. M. (University of Colorado, Center for Astrophysics and Space Astronomy); Norman, M. L. (University of California, San Diego, Center for Astrophysics and Space Sciences); Bryan, G. L. (University of Oxford)
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16. Questions: How Do Cluster Cores Evolve Cosmologically and Affect the Use of Clusters as Cosmological Probes?

US   How Evolution Can Affect the Use of Clusters As Cosmological Probes. XMM-Newton Observations of Distant Galaxy Clusters
Arnaud, M. (CEA/DSM/DAPNIA/Service d’Astrophysique)
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US   Galaxy Clusters As Cosmological Tools and Astrophysical Laboratories
Borgani, S. (Dipartimento di Astronomia, Università di Trieste)
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US   Cooling Cluster Cores and Cosmology
Reiprich, T. H. (University of Virginia); Sarazin, C. L. (University of Virginia)
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17. Meeting Summary

US   Meeting Summary: Cluster Cooling Flows Become Modest
Bregman, J. N. (University of Michigan)
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18. Conference Notes

US   Conference Note: A Taxonomy of Extended Radio Sources in Clusters of Galaxies
Kempner, J. C. (Harvard-Smithsonian Center for Astrophysics); Blanton, E. L. (University of Virginia); Clarke, T. E. (University of Virginia); Enßlin, T. A. (Max-Planck-Institut für Astrophysik); Johnston-Hollitt, M. (Leiden Observatory); Rudnick, L. (University of Minnesota)
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