We present a method for solving the light curve of an eclipsing binary system that contains a Cepheid variable as one of its components as well as the solutions for three eclipsing Cepheids in the
Shapes of RR Lyrae light curves can be described in terms of Fourier coefficients that past research has linked with physical characteristics such as luminosity, mass, and temperature.
In recent years a number of nonlinear codes have been discovered which have better error-correcting capabilities t h a n any known linear codes (e.g., Refs. 1 and 2).
We have identified a contribution to the ring current magnetic susceptibility of icosahedral C sub 60 which diverges paramagnetically as the relative strengths of the two inequivalent bonds of this
The magnetic deflection spectra of VCI sub 4 seeded into supersonic beams of the rare gases have been determined.
We present high resolution Bitter patterns which reveal the magnetic microstructure of the high T sub c superconductor Ba sub 2 YCu sub 3 0 sub 7, allowing the direct observation of vortices, and
usual cathode-ray type of tube and the very low currents obtainable therefrom prevent their use in most such proposals; their complicated guns and their large sizes are also undesirable features.
This paper documents a series of brief, strong (Ap/p=1), dynamic pressure oscillations which occurred in the region upstream of the earth's bow shock during a period of radial interplanetary magne
168 BELL SYSTEM TECHNICAL JOURNAL operating life satisfactory? Could its efficiency and output power be substantially increased?
The spontaneous polarization was measured for two chemically isomeric ferroelectric smectogens which have different phase sequences.
