Above the level of the photosphere is the stellar atmosphere.

This allowed the chemical composition of the stellar atmosphere to be determined.

Small carbon particles building up in the stellar atmosphere may be responsible.

Huge pulsations build up, which eventually become large enough to throw off the whole stellar atmosphere into space.

He also worked on the turbulence of stellar atmosphere and expanding shells around stars.

He specialized in spectroscopy and the study of stellar atmospheres.

It is often used to model radiative transfer, particularly in stellar atmospheres.

Scoops on the ship's leading edge sucked in samples of stellar atmosphere.

This would cause the stellar atmosphere swept up by the magnetic field to be flung outward.

Molecules may be found in many environments, however, from stellar atmospheres to those of planetary satellites.

The uppermost part of the stellar atmospheres forms a common envelope that surrounds both stars.

Stellar atmosphere, or stellar envelope, is the outermost region of a star.

We can imagine a region in the stellar atmosphere with a density lower than the surroundings, but with a higher radiation pressure.

The spectral signature of stars indicates the composition of the stellar atmosphere.

His main interests are stellar atmospheres, galactic chemical evolution and metal-poor stars.

C.T. Bolton was the first to develop a computer model for stellar atmospheres.

The motions of matter in stellar atmospheres.

This would "squeeze" the star, propelling stellar atmosphere through the polar magnetic nozzles.

A red supergiant like Betelgeuse will pulsate this way because its stellar atmosphere is unstable.

In astrophysics, photon diffusion occurs inside a stellar atmosphere.

Among his works were studies of stellar atmospheres and lunar occultations and eclipses.

Less dramatic, but equally convincing evidence is of large overabundances of specific stable elements in a stellar atmosphere.

If components in binary star systems are close enough they can gravitationally distort their mutual outer stellar atmospheres.

This research has application in understanding extreme plasma environments such as fusion tokamaks and stellar atmospheres.

He discovered new gaseous nebulas and the anomalous abundance of C in stellar atmospheres.