Detectable radio emission arises from stars across the entire H-R diagram, spanning virtually every stage of stellar evolution. The origin of stellar radio emission stems from a wide variety of physical processes, and observations of stars at radio wavelengths probe a broad range of astrophysical phenomena that cannot be studied by any other means.

This workshop will provide a forum for the presentation and discussion of the many advances in stellar and solar astrophysics recently (or soon to be) enabled by the latest generation of state-of-the-art radio facilities operating from meter to submillimeter wavelengths. We seek to bring together both observers and theorists to stimulate a lively exchange of ideas on how radio wavelength observations can provide new and unique insights into the workings of stars.

The workshop will focus on both hot and cool stars spanning the main sequence through post-main sequence evolutionary phases. We will also explore radio stars as probes of the Galaxy and the Galactic "ecosystem".

Invited review topics will include:

• An overview of stellar radio astronomy


• Radio emission at the bottom of the Main Sequence


• The Sun as a radio star


• The time domain in stellar physics


• Stellar wind theory


• The role of magnetic fields in stellar evolution


• Radio emission from evolved stars


• Circumstellar masers (theory and observation)


• Circumstellar chemistry


• White dwarf binaries


• Radio stars as players in our Galaxy


• Supernova progenitors


• Outlooks, controversies, and future challenges