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  3. Molecular Hydrogen in Space
  • Cited by 29
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    • Publisher:
      Cambridge University Press
      Publication date:
      04 August 2010
      06 November 2000
      ISBN:
      9780511564635
      DOI:
      https://doi.org/10.1017/CBO9780511564635
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      • Subjects:
      Physics and Astronomy, General and Classical Physics, Astrophysics
      Series:
      Cambridge Contemporary Astrophysics
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    • Selected: Digital
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    Subjects:
    Physics and Astronomy, General and Classical Physics, Astrophysics
    Series:
    Cambridge Contemporary Astrophysics
    Information

    Book description

    Molecular hydrogen is the most abundant molecule in the Universe. In recent years, advances in theory and laboratory experiments coupled with breakthrough observations with important new telescopes and satellites have revolutionized our understanding of molecular hydrogen in space. It is now possible to address the question of how molecular hydrogen formed in the early Universe and the role it played in the formation of primordial structures. This timely volume presents articles from a host of experts who reviewed this new understanding at an international conference in Paris. This book provides the first multi-disciplinary synthesis of our new understanding of molecular hydrogen. It covers the theory of the physical processes and laboratory experiments, as well as the latest observations. It will therefore be an invaluable reference for all students and researchers in astrophysics and cosmology.

    Reviews

    ‘… an invaluable reference for all students and researchers in astrophysics and cosmology.’

    Source: Europe & Astronomy

    ‘This book covers what seems like a very narrow subject - a conference on the behaviour of one molecule in the interstellar medium. But what a molecule! This conference proceedings, like all others, is a mixed bag of excellent reviews, reports of important and novel work, and of course more ephemeral recent results. its particular virtue is that the conference was set at an important time with results from ISO and now FUSE available, with major new calculations being completed, and with exciting new laboratory experiments being done … a pleasure to hold, and not wildly expensive.’

    Peter W. J. L. Brand Source: The Observatory

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    Contents

    Page 1 of 2

    Contents
    • The Interaction of H Atoms with Interstellar Dust Particles: Models
      pp 89-98
      • By V. Sidis, Laboratoire des Collisions Atomiques et Moléculaires (Unité Mixte de Recherche: CNRS – Université Paris Sud, No. 8625) Bâtiment 351, Université Paris Sud, 91405 Orsay Cedex, France, L. Jeloaica, Laboratoire des Collisions Atomiques et Moléculaires (Unité Mixte de Recherche: CNRS – Université Paris Sud, No. 8625) Bâtiment 351, Université Paris Sud, 91405 Orsay Cedex, France, A. G. Borisov, Laboratoire des Collisions Atomiques et Moléculaires (Unité Mixte de Recherche: CNRS – Université Paris Sud, No. 8625) Bâtiment 351, Université Paris Sud, 91405 Orsay Cedex, France, S. A. Deutscher, Laboratoire des Collisions Atomiques et Moléculaires (Unité Mixte de Recherche: CNRS – Université Paris Sud, No. 8625) Bâtiment 351, Université Paris Sud, 91405 Orsay Cedex, France
    • The Energetics and Efficiency of H2 Formation on the Surface of Simulated Interstellar Grains
      pp 99-106
      • By D. A. Williams, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, D. E. Williams, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, D. Clary, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, A. Farebrother, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, A. Fisher, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, J. Gingell, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, R. Jackman, Department of Electronic and Electrical Engineering, University College London, Gower Street, London WC1E 6BT, N. Mason, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, A. Meijer, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, J. Perry, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, S. Price, Department of Chemistry, University College London, Gower Street, London WC1E 6BT, J. Rawlings, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT

    Page 1 of 2

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