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The Art of Modeling Stars in the 21st Century (IAU S252)

The Art of Modeling Stars in the 21st Century (IAU S252)

The Art of Modeling Stars in the 21st Century (IAU S252)

L. Deng, National Astronomical Observatories, Chinese Academy of Sciences
K. L. Chan, Hong Kong University of Science and Technology
No date available
Hardback
9780521889834
Hardback

    Stellar models are the very basic building blocks with which we build up our knowledge of the Universe. New numerical experiments are heralding a new level of sophistication in our ability to model, and understand, how stars work. This volume provides an overview and the most recent advances in modelling of stellar structure and evolution. Modelling of stars relies on our understanding of the detailed physical processes happening in stars, and the most recent observations of stars made by modern large telescopes and current high technologies. IAU Symposium 252 presents the most recent developments in five key areas, including: improvements of the physical ingredients of stellar models; the evolution of low and intermediate mass stars; the evolution of massive stars; close binary evolution; and stellar physics in the era of very large telescopes. This overview of stellar research is at a level suitable for research astronomers and graduate students.

    • IAU S252 contains contributions from all of the many disciplines relevant to stellar evolution
    • Summarises the advances in our understanding of stellar evolution through modelling, due to new computing capabilities and better observations
    • Contains a full discussion of the key unresolved problems in the field

    Product details

    No date available
    Hardback
    9780521889834
    500 pages
    253 × 179 × 28 mm
    1.13kg
    100 b/w illus. 25 tables

    Table of Contents

    • Preface
    • Organizing committee
    • Conference participants
    • Session I. Updates of physical ingredients of stellar models Norbert Langer
    • Session II. Physical processes in stars Kwing-Lam Chan
    • Session III. From physics to stars, the progenitors of white dwarfs Vittorio Canuto and Jørgen Christensen-Dalsgaard
    • Session IV. From physics to stars, the progenitors of neutron stars and black holes Lee Anne Willson and Martin Asplund
    • Session V. Physics of stars in close binaries Philipp Podsiadlowski and Licai Deng
    • Session VI. New tools and future perspective Werner Däppen
    • Summary Norbert Langer
    • Author index
    • Subject index.
      Contributors
    • J. Ferguson, A. Dotter, M. Asplund, W. Däppen, D. Mao, E. Caffau, H.-G. Ludwig, J.-P. Zahn, D. R. Xiong, L. Deng, V. M. Canuto, Y. Cheng, A. Kučinskas, A. Stökl, S. Vauclair, M. Cantiello, N. Langer, J. Christensen-Dalsgaard, G. Houdek, D. O. Gough, G. Vauclair, J.-N. Fu, J.-E. Solheim, S.-L. Kim, M. Chevreton, N. Dolez, L. Chen, M. A. Wood, I. M. Silver, C. Charbonnel, S. Talon, A. Palacios, A. S. Brun, M. Yildiz, L. A. Willson, S. Kwok, F. Herwig, M. Mocák, E. Müller, T. Rauch, K. Werner, M. Ziegler, L. Koesterke, J. W. Kruk, P. Woitke, S. W. Campbell, J. C. Lattanzio, J. S. Vink, J. Krtička, L. Muijres, J. Puls, J. Kubát, Alex de Koter, M. Vick, G. Michaud, O. Richard, L. Siess, G. Hensler, G. Meynet, S. Ekström, C. Georgy, A. Maeder, R. Hirschi, R. Waldman, W. Wang, Z. Han, P. Podsiadlowski, Z. Li, S. E. de Mink, M. Cantiello, S.-Ch. Yoon, I. Brott, E. Glebbeek, M. Verkoulen, O. R. Pols, P. Lu, X. C. Meng, X. F. Chen, Z. Han, R. G. Izzard, M. Lugaro, S. E. de Mink, G. Q. Liu, M. Chávez, E. Bertone, A. Sadowski, J. Ziólkowski, K. Belczyński, T. Bulik, P. Kervella, S. K. Yi, Y.-C. Kim, P. Demarque, Y.-W. Lee, C. Meakin, F. Kupka

    • Editors
    • L. Deng , National Astronomical Observatories, Chinese Academy of Sciences
    • K. L. Chan , Hong Kong University of Science and Technology