... NEUTRON STAR: A celestial body hypothesized to occur in a terminal stage of stellar evolution, essentially consisting of a super dense mass of neutrons and having a powerful gravitational attraction from which only neutrinos and high-energy photons can ...

... Models of Mineral Dust Emission Eclipsing binary stars as cutting edge laboratories for astrophysics of stellar structure, stellar evolution and planet formation Unveiling first light from the infant Universe Simplifying Development and Deployment of High ...

... in the context e of stellar-dynamical problems rather than planetary evolution ... assumed that energy dissipation occurs in the process of stellar evolution ... V. V. and Larmor, J., The Kelvin-Poincare Problem of Stellar Evolution, Proc. Roy ...

... It is used to predict properties of high-redshift ob jects with evolutionary models, such as passive stellar evolution for galaxies. ...

... Exoplanet evolution - mass loss Stellar X-ray and EUV induced expansion of the upper atmospheres Stellar XUV luminosity energy deposition to upper atmospheres EXOBASE Exoplanet evolution - mass loss Soft X-ray and EUV induced expansion of the upper ...

... This astronomical instrument, designed to expand the knowledge of stellar evolution, scanned the local vicinity of our Milky Way galaxy and recorded the low-energy X-ray emanations believed to originate from the plasma remnants of an ancient supernova. ...

... No theory of stellar evolution offers any explanation for how a red star could become white in 2000 years, although much ...

... UVSTAR scientists also will observe the Io plasma torus around Jupiter, supernovae remnants and the hot blue stars within globular clusters, or the very dense clusters of stars that hold important clues about stellar evolution. ...