Structure and transport properties of amorphous aluminium silicates: computer simulation studies
The structure and transport properties of SiO2-Al2O3 melts containing 13 mol% and 47 mol% Al2O3 are investigated by means of
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The structure and transport properties of SiO2-Al2O3 melts containing 13 mol% and 47 mol% Al2O3 are investigated by means of
X-ray bursts from bright sources in globular clusters of our galaxy show that at least 11 (of a total 13)
We have derived a new photographic photometry and proper motions for 20000 stars with completeness to V = 18 in
We analyzed the Hipparcos astrometric observations of 47 stars that were discovered to harbor giant planets and 14 stars with
Recent theoretical work has made it plausible for neutron stars (NSs) to lose angular momentum via gravitational radiation on long
Due to the high-precision nature of the ASTROD (Astrodynamical Space Test of Relativity using Optical Devices) mission concept, the asteroid
The second of the annual BritGrav meetings on current research in Gravitational Physics in Britain took place at the School
In a recent article, Kim and Overhauser [Phys. Rev. B 47, 8025 (1993)] have found fault with the theory of
We present an algorithm for learning from unlabeled text, based on the Vector Space Model (VSM) of information retrieval, that
We report extensive multi-station photometry of TT Boo during its June 2004 superoutburst. The amplitude of the superoutburst was about
Dark matter appears in two forms as a consequence of the fluid mechanics of self-gravitational condensation. Condensation occurs primarily on
We first review reasons why dark matter is an interesting issue in connection with star clusters. Next we consider to
We outline a method to measure the detailed chemical composition of extragalactic (unresolved) globular clusters (GCs) from echelle spectra of
We illustrate the application of high precision Stromgren uvby photometry to open and globular clusters (GCs). It is shown how
Models applied to galaxies in equilibrium configuration are based on the solution of the collisionless Boltzmann equation and the Poisson
We present FIR and sub-mm images of the Crab nebula, taken with ISOPHOT on board ISO and with the SCUBA
Close to 70 radio pulsars have now been discovered in 23 globular clusters, with a record 22 pulsars observed in
We report here on two complementary population synthesis studies which relate directly to the formation and evolution of neutron star
The microlensing of background stars by compact objects in globular clusters is analyzed. The main strength of the proposed search
Fireballs are huge isotropic explosions models widely believed to explain Gamma Ray Burst, GRBs (Piran,1999); ever-new versions consider wide beamed
High resolution (R > 40 000) and high S/N spectra have been acquired with UVES on the VLT-Kueyen (Paranal Observatory,
We investigate the rotational velocities of early-type stars in the Sco OB2 association. We measure \vsini\ for 156 established and
This paper introduces Latent Relational Analysis (LRA), a method for measuring relational similarity. LRA has potential applications in many areas,
We present a method which provides some information on the possible binary nature on an appararently single star. The method