Winds of Stars and Exoplanets (IAU S370)

• Part I. Overview of winds of stars and exoplanets: 1. Winds and magnetospheres from stars and planets: similarities and differences; 2. Observations of winds and CMEs of low-mass stars; 3. Observations of outflows of massive stars; Part II. Observational evidence of winds: 4. Observations of planetary winds and outflows; 5. The effect of winds in red supergiants: modeling for interferometry; 6. The porous envelope and circumstellar wind matter of the closest carbon star, CW Leonis; 7. Is the magnetospheric accretion active in the Herbig Ae/Be stars?; 8. Short-term variations of surface magnetism and prominences of the young sun-like star V530 Per; 9. Water and silicon-monoxide masers monitored towards the 'water fountain' sources; 10. Weakening the wind with ULLYSES: Examining the Bi-stability jump; 11. Statistical properties of cold circumstellar envelops observed in NESS-NRO; 12. The origin of planetary winds; 13. Stellar wind from low-mass main-sequence stars: an overview of theoretical models; 14. The driving of hot star winds; 15. Slingshot prominences, formation, ejection and cycle frequency in cool stars; Part III. Physical ingredients of winds: 16. Effect of stellar flares and coronal mass ejections on the atmospheric escape from hot Jupiters; 17. Physics of the atmospheric escape driven by EUV photoionization heating: Classification of the hydrodynamic escape in close-in planets; 18. Discrete absorption components from 3-D spot models of hot star winds; 19. Hydrodynamic disk solutions for Be stars using HDUST; 20. Role of longitudinal waves in Alfvén-wave-driven solar/stellar wind; 21. ISOSCELES Grid of stellar atmosphere and hydrodynamic models of massive stars: The first results; 22. Quantification of the environment of cool stars using numerical simulations; 23. Hydrodynamic solutions of radiation driven wind from hot stars; 24. Gap opening by planets in discs with magnetised winds; 25. Solar wind and hydrologic cycle; 26. Magnetic confinement in the wind of low mass stars; 27. Clumping and X-rays in cool B supergiants; 28. Interaction between massive star winds and the interstellar medium; 29. Numerical modeling of galactic superwinds with time-evolving stellar feedback; Part IV. Flow-flow interactions: 30. Winds of OB stars: impact of metallicity, rotation and binary interaction; 31. X-ray view of colliding winds in WR 25; 32. Double tail structure in escaping atmospheres of magnetised close-in giant planets; 33. Shock breakout in winds of red supergiants: Type IIP supernovae; 34. On the making of a PN: the interaction of a multiple stellar wind with the ISM; 35. Role of planetary winds in planet evolution and population; 36. Size evolution and orbital architecture of KEPLER small planets through giant impacts and photoevaporation; Part V. Relevance of winds on stellar/planetary evolution: 37. Spin-down and reduced mass loss in early-type stars with large-scale magnetic fields; 38. Mass loss implementation and temperature evolution of very massive stars; 39. The evolution of atmospheric escape of highly irradiated gassy exoplanets; 40. The future of Jupiter-like planets around Sun-like stars: first steps; 41. Rapid orbital precession of the eclipsing binary HS Hydrae; 42. To the dynamics of the two-body problem with variable masses in the presence of reactive forces; 43; Evolution equations of the multi-planetary problem with variable masses; 44. Planet migration in accretion discs in binary systems; 45. Signatures of wind formation in optical spectra of precursors of planetary nebulae.

'The very diverse strands are, however, brought together in a comprehensive, magisterial survey by Stan Owocki of the physical processes driving the outflows from stars and planets - ranging from the CAK formalism of the line-driven winds of massive stars, through the solar corona and wind, spin-down, planetary winds and mass loss, followed by a discussion of magnetospheres of stars and planets. The proceedings continue with a section on observational evidence for winds, led by reviews on low-mass stars, high-mass stars, and planets … Conference proceedings containing reviews and short communications giving a snapshot of current work are often suggested as a good means for beginners to get started in a new field; the present volume gives entry to three.' Peredur Williams, The Observatory