Timing of the young pulsar J1907+0918
We have extensively searched for periodic signals in the area of the soft gamma-ray repeater SGR 1900+14, at 430 and
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A 140 Mpc Oscillation of the Abell Cluster Correlation Function
We have developed a parameter-independent method to detect local maxima of the two-point correlation function. By applying it to two
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Crystalline electron pairs
This is a nontechnical Perspective Commentary on the recent developments in cuprate STM and their ramifications for the theories of
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Electroweak Theory and the 1996/97 Precision Electroweak Data
We review the empirical evidence for the validity of the Standard Electroweak Theory in Nature. The experimental data are interpreted
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Fabrication of High Quality QC Films via the Route of the Amorphous Phase
We discuss the preparation of thin icosahedral films (Al-Cu-Fe and Al-Pd-Re) via the route of the amorphous (a-)phase which in
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New Pulsars from Arecibo Drift Scan Search
We report the discovery of 3 pulsars, PSR J0030+0451, PSR J0711+09, and PSR J1313+09 that were found in a three
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Peculiar Motions Of Clusters In The Perseus-Pisces Region
We present results of a new study of peculiar motions of 7 clusters in the Perseus-Pisces (PP) region, using the
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Photo-physical and nonlinear-optical properties of a new polymer: hydroxylated pyridyl para-phenylene
Photo-physical and nonlinear-optical properties of a new amphiphilic conjugated polymer: hydroxylated pyridyl para-phenylene (Py-PhPPP) both in CH2Cl2 solution and in
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Properties of CO Molecular Gas in IR Luminous Galaxies
We present the properties of the 12CO(1-0) and (3-2) line emission from the nuclei of 60 IR luminous SLUGS galaxies.
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Radio observations of the 33.8 ms X-ray pulsar SAX J0635+0533
The hard X-ray source SAX J0635+0533 shows pulsations at a period of 33.8 ms and is thought to be associated
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Slow pulsars from the STScI/NAIC drift scan search
The unique sensitivity of the Arecibo telescope at 430 MHz motivated a drift scan search of the visible sky divided
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Space-like meson electromagnetic form factor in a relativistic quark model
The space-like electromagnetic form factor is expressed in terms of the overlap integral of the initial and final meson wave
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Two-loop heavy top effects on precision observables and the Higgs mass
The electroweak corrections induced by a heavy top on the main precision observables are now available up to O(g^4 mt^2/mw^2).
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