Stellar Evolution, Atmospheres and Winds
The outside atmospheres of luminous cool huge stars and early type stars can be driven outward by radiation coming from the photosphere of the star. The radiation pressure forces the ounces outward, dragging ions along by viscous drag if the atmosphere is dense, thus creating a dust-driven wind.
- stellar wind bubbles
- Cosmic wind
Related Conference of Stellar Evolution, Atmospheres and Winds
December 12-13, 2024
4th International Conference on Applied Physics and Materials Science
Rome, Italy
June 19-20, 2025
8th International Conference on Astronomy, Astrophysics and Space Science
Budapest, Hungary
Stellar Evolution, Atmospheres and Winds Conference Speakers
Recommended Sessions
- Aeronautical and Aerospace Engineering
- Astrochemistry and Spectroscopy
- Astronomical Computing and Applications
- Astrophysics and Gravitational Waves
- Cosmic Microwave Background and Radiation
- Cosmology and Gravitational Physics
- Dark Matter, Dark Energy, and Black Holes
- Earth and Atmospheric science
- Electromagnetic radiation
- Exoplanets and Planetary Physics
- Galaxies and Big Bang Theory
- Neutrino and Nuclear Astrophysics
- Optical Astronomy and Optoelectronics
- Particle Physics and Higgs Boson
- Physics and Astronomy
- Planets, Comets, Asteroids and Dust
- Space Missions and Satellites
- Stars, Cool Dwarfs, Brown Dwarfs
- Stellar Evolution, Atmospheres and Winds
- Sun, Solar System and Extrasolar Planetary Systems
- Supernovae, Planetary Nebulae and Supernova Remnants
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