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Published online by Cambridge University Press: 26 May 2016
Speakers for this session were selected according to our perceptions about the frontier areas in dynamical atmospheres, the atmospheres of very cool stars, and stellar winds. This summary of posters and topics raised in the round table discussion opens with a brief summary of current issues in modeling pulsating stars and winds. Observational constraints are emphasized in Section 3. on “peeling the onion” of the atmosphere/wind structure. Section 4. covers a variety of methods for detecting and measuring stellar winds. The concluding remarks include some questions facing theorists and observers working in this field.