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 distinct 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 (AGB) star.

A bubble within the interstellar medium (ISM) formed from the outgoing stellar-wind is termed an asterosphere (the Sun's is called the heliosphere), and for very strong stellar winds, a stellar-wind bubble.

Stellar wind rates vary:


(stars)
Further reading:
https://en.wikipedia.org/wiki/Stellar_wind
https://en.wikipedia.org/wiki/Solar_wind
https://en.wikipedia.org/wiki/Superwind
https://en.wikipedia.org/wiki/Stellar-wind_bubble
https://dictionary.obspm.fr/index.php?showAll=1&formSearchTextfield=stellar+wind
https://astronomy.swin.edu.au/cosmos/s/stellar+winds
https://esahubble.org/wordbank/stellar-wind/
https://sites.astro.caltech.edu/~lah/ay102/slides/ay102_stellarwinds.pdf

Referenced by pages:
asymptotic giant branch (AGB)
atmospheric escape
aurora
brown dwarf (BD)
carbon star (C)
circumstellar envelope (CSE)
CMFGEN
falling evaporating body (FEB)
FIRE Simulations
gyrochronology
helium star
magnetic dipole braking
mass loading
mass loss
mass transfer
metallicity (Z)
Milky Way (MW)
P Cygni profile
Parker wind
planetary nebula (PN)
post-AGB star (pAGB)
presolar grain
protoplanetary nebula (PPN)
radiation belt
rocky planet
silicon monoxide (SiO)
solar wind
sound speed
star formation feedback
Stardust
stellar age determination
stellar evolution
stellar-mass black hole (stellar-mass BH)
symbiotic binary (SS)
T-Tauri star (TTS)
weathering
wind-momentum luminosity relationship (WLR)
Wolf-Rayet galaxy
Wolf-Rayet star
WR 140

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