Radiation pressure on condensing dust may cause this phenomenon in stars near the end of their lives.
Massive O and B stars may produce bubbles named after this phenomenon, filling huge cavities in the interstellar medium. Radiation pressure on condensing dust may cause this phenomenon in stars near the end of their lives. Wolf-Rayet stars have very strong ones of these, which causes them to lose relatively large amounts of their mass. The one produced by and named for the Sun is responsible for creating the overall shape of the Earth's magnetosphere and the auroras. Identify this phenomenon in which is a stream of particles released from the atmosphere of a star.
Massive O and B stars may produce bubbles named after this phenomenon, filling huge cavities in the interstellar medium.
{stellar wind} [anti-prompt on “solar wind”]