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  • © 2004

Magnetic Fields and Star Formation

Theory Versus Observations

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Table of contents (52 chapters)

  1. Front Matter

    Pages i-5
  2. Turbulence in the ISM

    1. Front Matter

      Pages 1-1
    2. A Review of the Theory of Incompressible MHD Turbulence

      • Benjamin D. G. Chandran
      Pages 17-28
    3. Magnetic Flux Transport in the ISM through Turbulent Ambipolar Diffusion

      • Fabian Heitsch, Ellen G. Zweibel, Adrianne D. Slyz, Julien E. G. Devriendt
      Pages 45-51
    4. High-Resolution Simulations of Nonhelical MHD Turbulence

      • N. E. L. Haugen, A. Brandenburg, W. Dobler
      Pages 53-60
    5. Scaling Relations of Supersonic Turbulence in Molecular Clouds

      • S. Boldyrev, P. Padoan, R. Jimenez, Å. Nordlund
      Pages 61-68
    6. Hydrodynamical Simulations of Molecular Dynamics in Supersonic Turbulent Flow

      • Georgi Pavlovski, Michael D. Smith, Mordecai-Mark Mac Low, Alexander Rosen
      Pages 69-75
    7. Structure of Molecular Clouds

      • Edith Falgarone, Pierre Hily-Blant, François Levrier
      Pages 89-101
    8. The Tiny-Scale Atomic Structure: Gas Cloudlets or Scintillation Phenomenon ?

      • S. Stanimirović, J. M. Weisberg, A. Hedden, K. Devine, T. Green, S. B. Anderson
      Pages 103-109
    9. BIMA and JCMT Spectropolarimetric Observations of the CO J = 2 − 1 Line Towards Orion KL/IRc2

      • J. M. Girart, J. S. Greaves, R. M. Crutcher, S.-P. Lai
      Pages 119-125
    10. The Measurement of the Orientation of the Magnetic Field in Molecular Clouds

      • Martin Houde, Ruisheng Peng, Hiroshige Yoshida, Roger H. Hildebrand, Thomas G. Phillips, C. Darren Dowell et al.
      Pages 127-134
  3. Formation of Structure and Fragmentation

    1. Front Matter

      Pages 135-135
    2. Fragmentation and Structure Formation

      • Enrique Vázquez-Semadeni
      Pages 137-142
    3. Turbulent Fragmentation and Star Formation

      • Javier Ballesteros-Paredes
      Pages 143-155
    4. Comments on Gravoturbulent Star Formation

      • Ralf S. Klessen
      Pages 165-173

About this book

Magnetic Fields play a key role in the physics of star formation on all scales: from the formation of the large complexes of molecular clouds to the formation of solar-like planetary systems. The plasma physics involved is non-linear and very complex, which requires the development of large numerical codes. An additional difficulty is that the detection and study of magnetic fields is not easy from an observational point of view, and therefore theoretical models cannot easily be constrained.

In the week from April 21st to 25th in 2003, a meeting was held on the Campus of the Universidad Complutense de Madrid (Spain) to join theoretical and observational efforts to address these issues. The objective was to define a set of relevant problems for the physics of star formation that can be properly addressed with the current or near-future instruments.

This book summarizes the results of this intensive week of work. The book is written in a comprehensive manner and reviews our current knowledge of the subject. It also represents an updated account of the ideas and thoughts of the scientists working in the field of Star Formation. The contributions are presented in six chapters which correspond to the six fundamental issues (sessions) on which the discussion was focused during the workshop: the physics of turbulence in the Interstellar Medium (ISM), the formation of structure in the ISM, the formation of stars within dense cores of molecular gas, the physics of accretion disks, the physics of outflows and their interaction with the ISM, and the interaction between the stellar magnetosphere and accretion disk.

Each chapter starts with a comprehensive summary written by one of the editors, which includes input from the contributions as well as the editor's own thoughts on the subject. For all these reasons the book is well-suited as a primer to introduce graduate students in the richness of this field of research.

Editors and Affiliations

  • Instituto de Astronomía y Geodesia (CSIC-UCM), Universidad Complutense de Madrid, Spain

    A. I. Gómez Castro

  • University of Massachussetts, Amherst, USA

    M. Heyer

  • Centro de Radioastronomía y Astrofísica, UNAM, Morelia, Michoacán, Mexico

    E. Vázquez-Semadeni

  • Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain

    R. Rebolo

  • Service d’Astrophysique, CEA-Saclay, Gif-sur-Yvette, France

    M. Tagger

  • McMaster University, Hamilton, Canada

    R. E. Pudritz

Bibliographic Information

  • Book Title: Magnetic Fields and Star Formation

  • Book Subtitle: Theory Versus Observations

  • Editors: A. I. Gómez Castro, M. Heyer, E. Vázquez-Semadeni, R. Rebolo, M. Tagger, R. E. Pudritz

  • DOI: https://doi.org/10.1007/978-94-017-0491-5

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: Springer Science+Business Media Dordrecht 2004

  • Hardcover ISBN: 978-1-4020-2159-6Published: 16 November 2004

  • Softcover ISBN: 978-90-481-6602-2Published: 17 September 2011

  • eBook ISBN: 978-94-017-0491-5Published: 12 June 2019

  • Edition Number: 1

  • Number of Pages: V, 516

  • Additional Information: Reprinted from Astrophysics and Space Science, 292:1-4

  • Topics: Astronomy, Observations and Techniques, Astrophysics and Astroparticles, Classical and Continuum Physics

Buy it now

Buying options

eBook USD 129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access