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Winds of Stars and Exoplanets (IAU S370)

Winds of Stars and Exoplanets (IAU S370)

Part of Proceedings of the International Astronomical Union Symposia and Colloquia

Stanley Owocki, Rachel Osten, Andrea Mehner, Leonardo Dos Santos, Gemma González-Torà, Hyosun Kim, Giovanni Pinzon, Cang Tianqi, Hiroshi Imai, Olivier Verhamme, Kei Amada, Daria Kubyshkina, Munehito Shoda, Andreas Sander, Simon Daley-Yates, Gopal Hazra, Hiroto Mitani, Florian Driessen, Catalina Arcos, Takeru Suzuki, Ignacio Araya, Judy Chebly, Michel Curé, Vardan Elbakyan, Xuguang Leng, Rose Waugh, Matheus Bernini-Peron, Jonathan Mackey, Ashkbiz Danehkar, Varsha Ramachandran, Bharti Arora, Aline Vidotto, Alak Ray, Arturo Manchado, Darius Modirrousta Galian, Pin-Gao Gu, Zsolt Keszthelyi, Gautham Sabhahit, Andrew Allan, Thomas Konings, Alisher Hojaev, Aigerim Ibraimova, Aiken Kosherbayeva, Sergei Popov, Kārlis Puķītis
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  • Date Published: September 2023
  • availability: In stock
  • format: Hardback
  • isbn: 9781009352789

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  • Winds form an integral part of astronomy – from regulating rotation of stars through enriching galaxies with fresh materials. Outflowing winds persist during the entire lives of stars and play a key role in shaping the exoplanet demographics we observe. In massive stars, their winds are a vital ingredient of their evolution, from the main sequence to the pre-supernova stage, determining black hole masses as measured from gravitational waves. In the case of low-mass stars, their winds dictate rotational evolution, which affect angular momentum distribution within the stellar interior and thus the generation of magnetic fields. In the case of planets, winds take the form of atmospheric escape, which can strongly affect their atmospheric evolution. IAU Symposium 370 brings together researchers on winds of exoplanets and stars, including the solar wind, to share insights into the physics and modelling tools used by these different communities.

    • Dedicated winds symposium features research on winds of close-in exoplanets (atmospheric escape), winds of low- and high-mass stars and the solar wind
    • Gives a broad insight into the work of different research communities
    • Part of the IAU's XXXIst General Assembly held in Busan, Korea, in August 2022
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    Reviews & endorsements

    '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

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    Product details

    • Date Published: September 2023
    • format: Hardback
    • isbn: 9781009352789
    • length: 300 pages
    • dimensions: 253 x 179 x 16 mm
    • weight: 0.63kg
    • availability: In stock
  • Table of Contents

    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.

  • Editors

    Aline Vidotto, Leiden Observatory, The Netherlands

    Luca Fossati, Space Research Institute, Austrian Academy of Sciences, Graz

    Jorick Vink, Armagh Observatory and Planetarium

    Contributors

    Stanley Owocki, Rachel Osten, Andrea Mehner, Leonardo Dos Santos, Gemma González-Torà, Hyosun Kim, Giovanni Pinzon, Cang Tianqi, Hiroshi Imai, Olivier Verhamme, Kei Amada, Daria Kubyshkina, Munehito Shoda, Andreas Sander, Simon Daley-Yates, Gopal Hazra, Hiroto Mitani, Florian Driessen, Catalina Arcos, Takeru Suzuki, Ignacio Araya, Judy Chebly, Michel Curé, Vardan Elbakyan, Xuguang Leng, Rose Waugh, Matheus Bernini-Peron, Jonathan Mackey, Ashkbiz Danehkar, Varsha Ramachandran, Bharti Arora, Aline Vidotto, Alak Ray, Arturo Manchado, Darius Modirrousta Galian, Pin-Gao Gu, Zsolt Keszthelyi, Gautham Sabhahit, Andrew Allan, Thomas Konings, Alisher Hojaev, Aigerim Ibraimova, Aiken Kosherbayeva, Sergei Popov, Kārlis Puķītis

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