Radio emission and mass loss rate limits of four young solar-type stars

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Radio emission and mass loss rate limits of four young solar-type stars

Aims. Observations of free-free continuum radio emission of four young main-sequence solar-type stars (EK Dra, p1UMa, ?1Ori, and ?1Cet) are studied to detect stellar winds or at least to place upper limits on their thermal radio emission, which is dominated by the ionized wind. The stars in our samp...

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Bibliographic Details
Main Authors:	Fichtinger, B., Güdel, M., Mutel, R., Hallinan, G., Gaidos, E., Skinner, S., Lynch, Christene, Gayley, K.
Format:	Journal Article
Published:	EDP Sciences 2017
Online Access:	http://hdl.handle.net/20.500.11937/69494

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