Determination of the chemical composition of stellar atmospheres
Chemical composition of stellar atmosphere related to galactic evolution
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Chemical composition of stellar atmosphere related to galactic evolution
History of theoretical research on stellar atmospheres, with bibliography
Inverse Compton effect in models of quasi-stellar objects demonstrated to be independent of magnetic field
Quasi-stellar object red shift correlation with radio magnitude
Stellar evolution model compared with observation to determine interior structure of real stars
Far UV radiation flux measurement by satellite- borne telescopic stellar spectrophotometer
Closed form solution expressing transonic flow in idealized stellar wind and spherical accretion problems including viscosity and thermoconductivity effects
Coincidences in measured positions of absorption lines in spectra of quasi-stellar objects
Red shift determinations for quasi-stellar radio sources using spectrographic techniques
Red shifts from absorption line spectra of quasi- stellar objects, discussing energy generation mechanism
Stellar pulsational instability phenomena calculated numerically for infinitesimal amplitude of central core motion
Mass dependence of behavior of stellar core undergoing gravitational collapse examined, using improved equation of state and mean free path for energy transfer
Motion in ternary stellar system consisting of central body and close and distant companions
Secular increase of stellar noncircular velocities in disk portions of galactic systems, noting gravitational disturbances
Optical polarimetric observations of quasi-stellar objects
Excited nuclei electromagnetic de-excitation rate by inelastic scattering in stellar particles calculated as function of temperature, density, transition energy and multipole functions
Energetic nuclear bombardment effects on stellar surface element abundance calculated with statistical theory in A magnetic variable star abundance anomaly
Abundance anomalies in stellar surface layers by proton and alpha particle bombardment caused nucleus breakdown and buildup to lower and higher mass numbers respectively