Effect of gravitational scalar field on high- density star structure.
Brans-Dicke theory of gravitational scalar field effect on structure of neutron cold spherical stellar model analyzed and compared with relativity theory
GRAVITATION THEORY↗
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Results for “Astronomical models”
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.
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Radar studies of the moon
Dielectric constants, composition, and depths of layers of moon based on two-layer lunar model using radar echoes
RADAR ECHO↗
A model of W Virginis with RV Tauri characteristics
Celestial model calculations for W Virginis star with RV Tauri characteristics
CELESTIAL BODY↗
Friedman cosmological models with both radiation and matter.
Friedman cosmological models describing spatially homogeneous and isotropic universe
INTERSTELLAR MATERIAL↗
A plasma model of quasars and radio galaxies
Models that treat events associated with quasi-stellar objects as plasma phenomena
ASTRONOMICAL MODEL↗
The Cosmic-Ray Electron Spectrum in a Disc-Halo Galactic Model
Cosmic-ray electron spectrum in disk-halo galactic model, studying inconsistencies in Ramaty and Lingenfelter analysis
ELECTRON SPECTRUM↗
Comments on Shklovsky's model for the X-ray source SCO XR-1.
Critical comments on Shklovsky model for newly identified X-ray source Sco XR-1
NEUTRON STAR↗
The linear star model and dynamical instability.
Pulsation properties of star models with linear density distribution, considering radial, adiabatic contraction and dynamical stability
DENSITY DISTRIBUTION↗
An interpretation of epsilon aurigae.
Rotating opaque gaseous disk model to explain contradictory behavior of binary Epsilon Aurigae found in photometric and spectroscopic observations
ROTATING DISK↗
Astrophysical evidence for the direct electron-neutrino weak interaction
Astrophysical evidence for direct electron- neutrino weak interaction - theoretical models of superluminous white dwarfs with and without neutrino emission process
NEUTRINO↗
Calculated physical properties of planets in relation to composition and gravitational layering.
Nonrotating, hydrostatic models of geochemically likely planets calculated using solar elemental abundances and equations of state for cold materials
ASTRONOMICAL MODEL↗
Numerical experiments with a one-dimensional model for a self-gravitating star system.
One-dimensional model of stellar system evolution, using computer to calculate minimum energy configuration
ENERGY DISTRIBUTION↗
Stellar evolution. IV - The evolution of a 9 solar masses star from the main sequence through core helium burning.
Evolution of 9 solar masses stellar model of population I initial composition from main sequence through core helium burning
HELIUM PLASMA↗
Cosmic rays in the interplanetary medium.
Streaming and spatial gradient equations of cosmic ray particles in interplanetary medium model, discussing Fokker-Planck equation and heliocentric field modulation
SOLAR WIND↗
The Influence of Water-Vapor Opacity and the Efficiency of Convection on Models of Late-Type Stars
Effective temperature for late type stars with or without water vapor opacity calculated for several masses, determining convective energy transport efficiency
ASTRONOMICAL MODEL↗
The distribution of gases in the protoplanetary nebula.
Solar system origin model successfully predicts relative terrestrial abundances of noble gases by taking into account ambipolar diffusion
PLANETARY ORIGIN↗
A model of quasi-stellar radio sources.
Theoretical model for quasars characterizes them as galactic flares, based on study of high energy phenomena associated with solar flares
QUASI-STELLAR RADIO SOURCE /QSO/↗
Models of stellar atmospheres
Stellar atmosphere models that assume interior energy sources, thermodynamic and mechanical equilibrium, and absorption of radiant energy only in continuous spectrum
THERMODYNAMIC EQUILIBRIUM↗