The intrinsic rotation of the Orion B stars with weak helium lines.
Intrinsic rotation of Orion B stars with weak He lines, discussing color-magnitude diagram
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.
Intrinsic rotation of Orion B stars with weak He lines, discussing color-magnitude diagram
Nonnewtonian intrinsic viscosity of polymer solutions
Intrinsic brightness of comet Ikeya in comparison with nearby stars
Photoconductivity of X-ray irradiated cadmium sulfide single crystal and annealing of intrinsic defects
Production and annealing of intrinsic defects in X-ray irradiated CdS single crystals
Production and annealing of intrinsic defects in X-ray irradiated cadmium sulfide single crystals
Structural model of lunar mantle based on lunar intrinsic infrared radiation
Intrinsic magnetic dipole moment of Venus based on absence of radiation belt electrons
Electromagnetic field behavior near conducting wedge edge in contact with uniaxial plasma, noting intrinsic loss without surface waves
Invalidity of Pagel method for intrinsic and interstellar reddening for peculiar objects, discussing excitation mechanism for forbidden lines of ionized Fe for Eta Carinae
Intrinsic transport theorem for electrodynamics of continuous media, using Cartan method of exterior differential forms
Intrinsic mechanism in gracilis muscle for autoregulation of blood flow
Comparing intrinsic efficiencies of spherical NaI /Tl/ detectors with efficiencies of cylindrical NaI/Tl/ detectors
Reddening effects in determining intrinsic color of supergiant and cepheid variable stars
The intrinsic thermal radiation of the moon is an indicator of the temperature regime of the lunar surface, its physical conditions and structure, as indicated by data from Luna 9 and 13, as well as Surveyor 1 to 7.
The first part of the present theory is devoted to the derivation of a Fokker-Planck equation. The eddies smaller than the hydrodynamic scale of the diffusion cloud form a diffusivity, while the inhomogeneous, bigger eddies give rise to a nonuniform migratory drift. This introduces an eddy-induced shear which reflects on the large-scale diffusion. The eddy-induced shear does not require the presence of a permanent wind shear and is intrinsic to the diffusion. Secondly, a transport theory of diffusivity is developed by the method of repeated-cascade and is based upon a relaxation of a chain of memories with decreasing information. The full range of diffusion consists of inertia, composite, and shear subranges, for which variance and eddy diffusivities are predicted. The coefficients are evaluated. Comparison with experiments in the upper atmosphere and oceans is made.
The intrinsic phase-dependent linear polarization of two magnetic Ap stars is studied. The polarization characteristics in a broad blue filter band and in the ultraviolet are outlined, and the mechanisms of polarization are examined. The blue band polarization of 53 Cam (corrected by removing the stellar component) is found to be compatible with an oblique rotator whose angular parameters are in essential agreement with those deduced by Landstreet (1970) and by Huchra (1972).
The X-ray spectrum of Hercules X-1 was observed in the energy range 2-24 keV with sufficient temporal resolution to allow detailed study of spectral correlations with the 1.24 sec pulse phase. A region of spectral hardening which extends over approximately the 1/10 pulse phase may be associated with the underlying beam. The pulse shape stability and its asymmetry relative to this intrinsic beam are discussed.