Any stream of gas flowing outward from a star, including the very rapid winds from hot, luminous stars; the intermediate- velocity, rarefied winds from stars like the sun; and the slow, dense winds from cool supergiant stars
the ejection of gas off the surface of a star. Many different types of stars, including our Sun, have stellar winds; however, a star's wind is strongest near the end of its life when it has consumed most of its fuel. (See also text in StarForm and StarDeath.)
is the flow of material from a star to the Galaxy. In the electric star the stellar wind exists as one means of the star accumulating charge from the nearly "empty" space which surrounds it. By sending electron-deficient atoms to the Galaxy the star gains electrons relative to the material it contains. From the few stellar winds that have been measured, it seems as if the mass loss increases as the square root of the luminosity. In terms of the electric star model presented here, it is tempting to think that luminosity varies as the square of the star-to-galaxy current. There is some evidence that mass loss is enhanced when a close companion is present (Hutchings).
a constant stream of sub-atomic particles moving at faster than the escape velocity of the star's gravitational field
a steady stream of electrons and protons that flows off the surface of a star into space
The ejection of gas from the surface of a star. Many different types of stars, including our Sun, have stellar winds. The stellar wind of our Sun is also known as the Solar wind. A star's stellar wind is strongest near the end of its life when it has consumed most of its fuel.
The outflow of gas, sometimes at speeds as high as hundreds of kilometers per second, from a star.
Stellar wind is gas that is ejected from the surface of a star (including the Sun). Older (evolved) stars give off stronger stellar winds.
a stream of particles flowing from a star (like the solar wind, but around a star other than the Sun)