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

descriptionPublicationkeyboard_double_arrow_right Article , Conference object , Preprint , Other literature type 01 Jan 2018Embargo end date: 01 Jan 2018Publisher:arXiv

Authors: Forbrich, Jan; Williams, Peter K. G.; Drabek-Maunder, Emily; Howard, Ward; Jardine, Moira; Matthews, Lynn; Moschou, Sofia; +8 Authors

doi: 10.48550/arxiv.1811.03616 , 10.5281/zenodo.1476616 , 10.5281/zenodo.1476617

arXiv: 1811.03616

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

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Abstract

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.

Splinter session summary, to appear in the proceedings of the 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (ed. S. J. Wolk)

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Keywords

Astrophysics - Solar and Stellar Astrophysics, FOS: Physical sciences, Solar and Stellar Astrophysics (astro-ph.SR)

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