stellar wind

He could almost imagine the stellar winds on his face.

Its stellar wind is over 10 billion times stronger than the Sun's.

The majority of the star's mass was shed, most likely as a stellar wind.

We can't beam down because of all that radiation and stellar wind.

Much of this radiation is absorbed by the primary stellar wind.

The way we're coming in, there's enough stellar wind that it's feasible we couldn't read them yet.

Stellar wind is gas being thrown off from the upper atmosphere of a star.

These reached mass loss rates much higher than stellar winds would normally allow.

This produced a faster stellar wind which compressed the gas.

The magnetic field of a star interacts with the stellar wind.

These winds can form stellar wind bubbles dozens of light years across.

Other stars have much stronger stellar winds that result in significantly higher mass loss rates.

The strong stellar winds at this time remove most of the remaining nebula.

This shell was likely created by a strong stellar wind from the progenitor star.

These originate in the stellar wind escaping from the giant star.

There are two classic explanations for the mass loss of stars by stellar winds.

Its intense stellar winds have been measured on the order of 100 km/s.

Their ages are based partly on their strong stellar winds.

The collision of the stellar winds from this pair makes the system a strong X-ray source.

Only very massive stars greater than 10 times the sun's mass have stellar winds throughout their lifetimes.

Stars slowly lose mass by the emission of a stellar wind from the photosphere.

Such cavities might be created by stellar winds and supernovae.

The important difference is that the stellar wind is atomic nuclei.

If he gets swept away by a stellar wind or something, the first we hear is when he doesn't call in."

For stars, this is typically the boundary between their stellar wind and the interstellar medium.