The continuous flow of gas from the surface of a star into space. It is
most intense toward the beginning and the end of a star's life, as exemplified
by T Tauri stars, on the one hand, and red
giants and supergiants, on the
|Hubble Space Telescope image of a bubble-like cavity,
called N44F, 35 light-years in diameter, which is being inflated by
a stellar wind from a very hot star once buried inside a cold dense
cloud. The central star in N44F is ejecting mass at a rate greater
than a 100 million times that in the solar wind. The particles in
this stellar wind move at 7 million kilometers per hour, compared
with about 1.5 million km per hour in the case of the Sun. N44F is
located about 160,000 light-years away in the Large Magellanic Cloud.
Credit: NASA, ESA, Y. Nazé (University of Liège, Belgium)
and Y.-H. Chu (University of Illinois, Urbana).
Among the most extreme stellar winds, resulting in a loss of 10-6
solar mass or more per year, are those that occur in X-ray
binaries, in which in O and B stars are being stripped by a compact
companion (either a neutron star or a black hole).
During their time on the main sequence,
most stars blow a very modest stellar wind; in the Sun's case this amounts
to a mass loss of only about 10-14 solar mass per year (see solar
wind). Stellar winds represents an important mechanism by material is
returned to the interstellar medium to be recycled
as a new generation of stars.