The Relevance of Magnetic Fields to Stars and Accretion Disks

  • G. Belvedere
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 156)


As clearly stated in the Introductory talk, during the Opening Ceremony, the significance of the Conference was in gathering together scientists actively working in different research fields with a common background of expertises, in order to highlight a varied but in some sense unified scenario of the interaction of rotation, turbulence and magnetism in different astrophysical systems, with primary interest in stars and accretion disks and specific regard to objects and topics ranging from star formation, solar and stellar magnetic activity, and close binaries, to neutron stars, X-ray galactic sources and active galactic nuclei (AGN).


Black Hole Accretion Disk White Dwarf Aetive Galactic Nuelei Dynamo Model 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • G. Belvedere
    • 1
  1. 1.Istituto di AstronomiaUniversità di CataniaItaly

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