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Conference Paper

A model for the decline of coronal X-ray emission of cool giant stars

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons103972

Holzwarth,  Volkmar
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104196

Schüssler,  Manfred
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104218

Solanki,  Sami K.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Holzwarth, V., Schüssler, M., & Solanki, S. K. (2001). A model for the decline of coronal X-ray emission of cool giant stars. In G. Mathys, S. K. Solanki, & D. T. Wickramasinghe (Eds.), Magnetic Fields Across the Hertzsprung-Russell Diagram (pp. 259-262). San Francisco/CA: Astronomical Society of the Pacific.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-E7C1-1
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