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Warped Disks and Inclined Rings around Galaxies

Warped Disks and Inclined Rings around Galaxies

Warped Disks and Inclined Rings around Galaxies

Stefano Casertano, University of Pittsburgh
Penny D. Sackett, University of Pittsburgh
Franklin H. Briggs, University of Pittsburgh
November 2006
Paperback
9780521031639
$46.99
USD
Paperback
USD
Hardback

    Most galaxies lie in clusters, where tidal interactions are a significant force. Tidal and dynamical interactions and the features they cause in galaxies are important to the study of galactic evolution. For example, a large amount of data has been collected on dust-lane ellipticals, polar-ring galaxies, spirals with extended warps, and galaxies with inclined HI rings or unusual "tails." This book is a record of a meeting held at the University of Pittsburgh that provided an informal, yet focused environment for the interaction of astronomers who have addressed these questions with a wide variety of skills, techniques, and points of view.

    Reviews & endorsements

    "The papers, intended for graduate students and professional astronomers, are unusually well written. The reader will be grateful that the book is well indexed and will also appreciate the transcription of the workshop's wrap-up discussion." Science Books & Films

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    Product details

    November 2006
    Paperback
    9780521031639
    312 pages
    243 × 168 × 16 mm
    0.509kg
    2 b/w illus.
    Available

    Table of Contents

    • Preface
    • Acknowledgements
    • Workshop participants
    • Group photograph
    • 1. The intergalactic HI supply F. Briggs
    • 2. Neutral gas infall into NGC 628 J. Kamphuis and F. Briggs
    • 3. VLA HI observations of the radio galaxy Centaurus A J. M. van der Hulst, J. H. van Gorkom, A. D. Haschick and A. D. Tubbs
    • 4. A geometric model for the dust-band of Centaurus A R. A. Nicholson, K. Taylor and J. Bland
    • 5. The circumgalactic ring of gas in Leo S. E. Schneider
    • 6. Using gas kinematics to measure M/L in elliptical galaxies T. de Zeeuw
    • 7. Velocity fields of disks in triaxial potentials P. J. Teuben
    • 8. Modeling the atomic gas in NGC 4278 J. F. Lees
    • 9. A few statistics from the catalog of polar-ring galaxies B. C. Whitmore
    • 10. Dynamics of polar rings L. S. Sparke
    • 11. Mergers and the structure of disk galaxies L. Hernquist
    • 12. Formation of polar rings H.-W. Rix and N. Katz
    • 13. Gas-dynamical models of settling disks D. Christodoulou and J. E. Tohline
    • 14. Evolutionary processes affecting galactic accretion disks T. Steiman-Cameron
    • 15. Particle simulations of polar rings T. Quinn
    • 16. A bending instability in prolate stellar systems D. Merritt
    • 17. The Milky Way: lopsided or barred? K. Kuijken
    • 18. Merger origin of starburst galaxies L. Hernquist
    • 19. Warped and flaring HI disks A. Bosma
    • 20. Behaviour of warps in extended disks F. Briggs and J. Kamphuis
    • 21. Observational constraints for the explanation of warps E. Battaner, E. Florido, M.-L. Sanchez-Saavedra and M. Prieto
    • 22. Warps in S0s: observations versus theories G. Galletta
    • 23. Warps and bulges J. Pitesky
    • 24. Time evolution of galactic warps P. Hofner and L. S. Sparke
    • 25. Are warps normal modes? S. Casertano
    • 26. Disk warping in a slewing potential E. C. Ostriker
    • 27. Concluding discussion Moderator: K. C. Freeman
    • Name index
    • Object index
    • Subject index.
      Contributors
    • F. Briggs, J. Kamphuis, J. M. van der Hulst, J. H. van Gorkom, A. D. Haschick, A. D. Tubbs, R. A. Nicholson, K. Taylor, J. Bland, S. E. Schneider, T. de Zeeuw, P. J. Teuben, J. F. Lees, B. C. Whitmore, L. S. Sparke, L. Hernquist, H.-W. Rix, N. Katz, D. Christodoulou, T. Steiman-Cameron, T. Quinn, D. Merritt, K. Kuijken, A. Bosma, E. Battaner, E. Florido, M.-L. Sanchez-Saavedra, M. Prieto, G. Galletta, J. Pitesky, P. Hofner, S. Casertano, E. C. Ostriker, K. C. Freeman

    • Editors
    • Stefano Casertano , University of Pittsburgh
    • Penny D. Sackett , University of Pittsburgh
    • Franklin H. Briggs , University of Pittsburgh