Binary sequences with specified correlation properties
Binary sequences with specified correlation properties
Seguin, G.↗
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Evidence for a collapsar in the binary system epsilon Aur
Black hole model accounting for epsilon Aur eclipsing binary secondary component observations
Cameron, A. G. W.↗
Collapsars, infrared disks and invisible secondaries of massive binary systems
Epsilon Aur eclipsing binary primary star mass and evolutionary stage considered to interpret secondary
Stothers, R.↗
A three-element model for binary prediction
Three element model for choice behavior binary prediction consisting of logical, experiential and error components
Hartley, R. E.↗
Binary sequences with a relaxed Barker criterion
Binary sequences with relaxed Barker criterion, examining correlation coefficients
Seguin, G.↗
A model atmosphere analysis of the binary 112 Herculis
Binary star 112 Herculis elemental abundances by atmospheric model analysis of spectra
Aller, L. H.↗
Intermolecular forces in globular molecules. VIII - Binary gaseous mixtures
Spherical shell potential extension to shells of differing diameters for intermolecular forces in globular molecules, considering binary gaseous mixtures
De Rocco, A. G.↗
Bootstrap hybrid decoding for symmetrical binary input channels
Hybrid decoding technique for symmetrical binary input channels, using bootstrap algorithm across convolutionally encoded information streams
Cocke, J.↗
On the formation of a neutron star in a close binary system
Neutron star formation from supernova explosion in close binary system
Kondo, Y.↗
The application of Kirkwood expansions to binary interstitial solutions
Binary interstitial solid solutions thermodynamic properties calculation with Kirkwood expansion, allowing crystal first order partition function measurement without degeneracy error
Alex, K.↗
The weight enumerators for several classes of subcodes of the 2nd order binary Reed-Muller codes
Explicit formulas for Euclidean geometry and Berlekamp subcodes weight enumerators for second order binary Reed-Muller codes
Kasami, T.↗
Comments on 'Effects of band limiting on the detection of binary signals'
Critique of paper on additional signal power for optimum performance of PCM binary signal detection under channel band limiting effect in white noise
Shehadeh, N. M.↗
Monochromatic reflection effect of close binary stars
Close binary stars monochromatic reflection effect calculation, using surface temperature distribution model
Chen, K.-Y.↗
An analytic model of eclipsing binary star systems
Analytical model of eclipsing binary star systems, testing validity through numerical integration error analysis
Wood, D. B.↗
Decoding binary block codes on Q-ary output channels
Error correcting binary block code decoding on Q-ary output channels /weighted erasure decoding/, considering applications
Weldon, E. J., Jr.↗
Correlations among the parameters of the spherical model for eclipsing binaries
Correlation coefficients were computed to investigate the parameters for describing the spherical model of an eclipsing binary system. Regions in parameter hyperspace were identified where strong correlations exist and, by implication, the solution determinacy is low. The results are presented in tabular form for a large number of system configurations.
Sobieski, S.↗
Alloy softening in binary molybdenum alloys
An investigation was conducted to determine the effects of alloy additions of Hf, Ta, W, Re, Os, Ir, and Pt on the hardness of Mo. Special emphasis was placed on alloy softening in these binary Mo alloys. Results showed that alloy softening was produced by those elements having an excess of s+d electrons compared to Mo, while those elements having an equal number or fewer s+d electrons than Mo failed to produce alloy softening. Alloy softening and hardening can be correlated with the difference in number of s+d electrons of the solute element and Mo.
Stephens, J. R.↗
Alloy hardening and softening in binary molybdenum alloys as related to electron concentration
An investigation was conducted to determine the effects of alloy additions of hafnium, tantalum, tungsten, rhenium, osmium, iridium, and platinum on hardness of molybdenum. Special emphasis was placed on alloy softening in these binary molybdenum alloys. Results showed that alloy softening was produced by those elements having an excess of s+d electrons compared to molybdenum, while those elements having an equal number or fewer s+d electrons that molybdenum failed to produce alloy softening. Alloy softening and alloy hardening can be correlated with the difference in number of s+d electrons of the solute element and molybdenum.
Stephens, J. R.↗