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
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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
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- Electromagnetic radiation
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- Planets, Comets, Asteroids and Dust
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- Sun, Solar System and Extrasolar Planetary Systems
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