The 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Published November 1, 2018 | Version v1
Conference paper Open

Meter- to Millimeter Emission from Cool Stellar Systems: Latest Results, Synergies Across the Spectrum, and Outlook for the Next Decade

Creators

  • 1. Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK
  • 2. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
  • 3. Royal Observatory Greenwich, Blackheath Ave, London SE10 8XJ, UK
  • 4. Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255, USA
  • 5. Centre for Exoplanet Science, SUPA, School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK
  • 6. MIT Haystack Observatory, 99 Millstone Road, Westford, MA 01886, USA
  • 7. Department of Physics and Astronomy, University of Iowa, 203 Van Allen Hall, Iowa City, IA, 52242, USA
  • 8. Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands
  • 9. National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA
  • 10. Sydney Institute for Astronomy (SIfA), School of Physics, The University of Sydney, NSW 2006, Australia
  • 11. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
  • 12. University of Vienna, Department of Astrophysics, T�rkenschanzstrasse 17, 1180 Vienna, Austria

Description

Radio observations of cool stellar systems provide unique information on their magnetic fields, high-energy processes, and chemistry. Buoyed by powerful new instruments (e.g. ALMA, JVLA, LOFAR), advances in related fields (e.g., the Gaia astrometric revolution), and above all a renewed interest in the relevant stellar astrophysics, stellar radio astronomy is experiencing a renaissance. In this splinter session, participants took stock of the present state of stellar radio astronomy to chart a course for the field's future.

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Cool_Stars_20_radio_splinter_proceedings.pdf

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