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We present broadband and narrowband Hubble Space Telescope images of the central region of the heavily disturbed Virgo cluster galaxy
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This paper will present the exact solution for the stress-energy tensor of a spherical matter shell of finite thickness that
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We have used the vectorised and parallelised magnetohydrodynamics code NIRVANA on the NEC SX-5 and the new SX-6 installation in
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We calculate the expected envelope of emission for relativistic shells under the assumption of local spherical symmetry. Gamma-Ray Burst envelopes
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We present a new complementary strategy to quasicrystalline structure determination: The local atomic structure of simple icosahedral (si) Ho11Mg15Zn74 [a(6D)=5.144(3)A]
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We discuss the possibility of explaining the observation of ultra-high-energy cosmic rays with energy above the GZK cutoff, saving the
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Lumbar Support - Backrest - Driver Seat (Remove and Replace) 2017-2023 Model 3 Service ManualTorque CalculatorVideo LibraryMenuTorque CalculatorVideo Library2026-08-09 Lumbar
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Lumbar Support - Back Rest - Front Passenger Seat (Remove and Replace) 2017-2023 Model 3 Service ManualTorque CalculatorVideo LibraryMenuTorque CalculatorVideo
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By LDA+U method with spin-orbit coupling (LDA+U+SO) the magnetic state and electronic structure have been investigated for plutonium in δand
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arxiv
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The well-known light minima of stars with the R Coronae Borealis variability are caused by the formation of an additional
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An isolated, spherically-symmetric, self-gravitating, collisionless system is always a polytrope when it reaches equilibrium (Nakamura 2000). This strongly suggests as
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The interaction of an expanding Pair-Electromagnetic pulse (PEM pulse) with a shell of baryonic matter surrounding a Black Hole with
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A new synthesis of the principles of relativity and quantum mechanics is developed by replacing the Poincaré group for the
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2017-2023 Model 3 Service ManualTorque CalculatorVideo LibraryMenuTorque CalculatorVideo Library2026-08-09 Post Guide - Headrest - Front Passenger Seat (Remove and Replace)
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dennis
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In many models of Gamma-Ray Bursts (GRBs) relativistic shells are responsible for the overall envelope of emission. We use kinematics
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arxiv
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Photoionisation of an atom by X-rays usually removes an inner-shell electron from the atom, leaving behind a perturbed "hollow ion"
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Recent LEP results on single and pair production of neutral electroweak gauge bosons are reviewed. QED and Electroweak gamma-e Compton
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[condensed] A new scenario is presented for the production of Na23 in asymptotic giant branch (AGB) stars. The scenario takes
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High resolution spectroscopic observations of Seyfert galaxies with Chandra and XMM-Newton allows us to study the detailed ionization and thermal
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We present initial results of a spectroscopic study of the Pistol and of the cocoon stars in the Quintuplet Cluster.
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Excess reddened optical emission has been measured in the power-law decay afterglow light curves of several GRBs some tens of
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Recent observations suggest that $γ$-ray bursts (GRBs) and their afterglows are produced by jets of highly relativistic cannonballs (CBs), emitted
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We study the formation and stability of regular black holes by employing a thin shell approximation to the dynamics of
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arxiv