Astrophysics (Index)About

stellar wind

(gas or plasma emanating from a star)

Stellar wind is outward-moving gas from a stellar atmosphere, presumed steadier than bursts. It is the analog of solar wind for other stars, but for other types of stars, the makeup and other characteristics of the wind can vary. For example, massive stars tend to have much stronger stellar wind, to the point of emitting much more of their mass over a much shorter lifetime. The term superwind refers to an extreme wind in a very late phase of an asymptotic giant branch star.

Further reading:

Referenced by pages:
asymptotic giant branch (AGB)
atmospheric escape
brown dwarf (BD)
carbon star
falling evaporating body (FEB)
star formation feedback
FIRE Simulations
HI supershell
mass loading
mass loss
Milky Way
P Cygni profile
planetary nebula (PN)
Proxima b
rocky planet
solar wind
sound speed
stellar age determination
stellar evolution
symbiotic binary (SS)
Wolf-Rayet galaxy
Wolf-Rayet star