Explore: Stellar Physics

astrophysicists) Neutrino astronomy – Observing low-mass stellar particles Timeline of gravitational physics and relativity Timeline of knowledge about galaxies

In astrophysics, stellar nucleosynthesis is the creation of chemical elements by nuclear fusion reactions within stars. Stellar nucleosynthesis has occurred

The stellar physics department is focused on research of stars, primarily hot stars (class B), models of stellar atmospheres, dynamics of stellar winds

resulting in thunderstorms. Natural convection also plays a role in stellar physics. Convection is often categorised or described by the main effect causing

Stellar structure models describe the internal structure of a star in detail and make predictions about the luminosity, the color and the future evolution

for developing ideas on stellar physics. In 1926, in his book The Internal Constitution of the Stars he explained the physics of how stars fit on the

A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars

A stellar core is the extremely hot, dense region at the center of a star. For an ordinary main sequence star, the core region is the volume where the

the cords' material and tension. Similarly, stellar pulsation modes are characteristic of global stellar properties and of the internal physical conditions

Related to Stellar properties, Pages using the word stellar in a physics context. Stellar aberration Stellar age estimation Stellar archaeology Stellar astronomy