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VLA Observations of Quiescent and Flare Microwave Emission from Late-Type Stars: A Unique Probe of Coronal Magnetic Fields
Published online by Cambridge University Press: 04 August 2017
Extract
The high sensitivity and angular resolving power of the VLA permits observations for the first time of the steady (quiescent) microwave emission from stellar coronae as well as detailed studies of stellar flares. Gary and Linsky (1981) first detected steady 6 cm emission from χ1 Ori (GO V) and UV Cet (M5.6e V), and Topka and Marsh (1982) subsequently detected quiescent emission from both components of EQ Peg (dM3.5e + dM4.5e).
- Type
- IV. The Role of Magnetic Fields in the Structure and Energy Balance of Stellar Atmospheres
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- Copyright © Reidel 1983