Galactic H II regions and the luminosity of the galaxy in 12.8-micron radiation.
Luminosity of galactic disk in 12.8 micron radiation, obtaining from volume integral stellar photon flux density and thermal radio emission rate
SEARCH · Search NASA
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.
Luminosity of galactic disk in 12.8 micron radiation, obtaining from volume integral stellar photon flux density and thermal radio emission rate
Determination of helium abundances, and luminosity of horizontal branch stars
Globular cluster M13 luminosity function by reflecting telescope plates star counts, obtaining evolutionary stages lifetime and He core mass
Auroral band electron energy spectra, electron number density, ionization and luminosity obtained from rocket measurements
Bolometric luminosity-red shift relations of Friedmann dust universes corrected for inhomogeneities, using locally inhomogeneous Swiss cheese models
Long period, semiregular, and irregular high luminosity variable stars
High luminosity white dwarfs possible evolution from planetary nebulae, discussing plasma neutrino processes
Luminosity criteria in O stars via narrow band photoelectric photometry suggesting VI Cygni proximity
Luminosity effects in Balmer lines of early type stars, noting H alpha equivalent width decrease
Time constant loci and theoretical luminosity functions for various compositions and ages of metal poor globular clusters
High luminosity M type star photometry, determining supergiant intrinsic properties, interstellar extinction mean law and galactic evolution
Solar activity and planetary luminosity
Artificial meteors ablation and luminosity measurements, using ballistic range shadowgraph and radiometric equipment for velocity history, shock wave formation and mass loss process
Neutrino luminosity in strongly magnetized degenerate relativistic electron gas plasma from URCA energy loss rate calculations
Individual M-type red supergiants luminosity, masses and periodicities based on cluster membership and pulsational Q value
High luminosity G supergiants at 0.4-18 micron wavelengths showing intense silicate emission shell
The solar neutrino problem is considered, giving attention to the experiments conducted to detect solar neutrinos and the possible reasons for the failure to detect neutrinos emitted from the solar interior. According to one suggestion the core of the sun is in a temporarily expanded condition with a consequent lowering in the emitted neutrino flux from the center of the sun. A possible mechanism that could provide the core expansion is proposed. The effects of mixing reactions in the solar interior are discussed together with variations in solar luminosity which might be responsible for the occurrence of the periods of glaciation.