Shell-effects in heavy alkali-metal nanowires
We supplement our previous observations of the shell effect in alkali-metal nanowires (Li, Na, K) with data extended to the
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Answer sourceWe supplement our previous observations of the shell effect in alkali-metal nanowires (Li, Na, K) with data extended to the
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Shell signs in the hydrogen-line spectrum of some lambda Bootis-type stars
The hydrogen-line spectrum of eight lambda Boo type stars is studied. The observed H_delta and H_gamma profiles are compared with
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2-D Radiation Transfer Model of Non-Spherically Symmetric Dust Shell in P roto-Planetary Nebulae
We have fitted the HST images and the spectral energy distributions (SEDs) of three proto-planetary nebulae (PPN) with a 2-D
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76 mas speckle-masking interferometry of IRC+10216 with the SAO 6m telescope: Evidence for a clumpy shell structure
We present the first K'-band image of the carbon star IRC+10216 with 76 mas resolution. The diffraction-limited image was reconstructed
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Algorithm for generating quasiperiodic packings of icosahedral three-shell clusters
The strip projection method is the most important way to generate quasiperiodic patterns with predefined local structure. We have obtained
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Algorithm for Generating Quasiperiodic Packings of Multi-Shell Clusters
Many of the mathematical models used in quasicrystal physics are based on tilings of the plane or space obtained by
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Analysis of a Shell System in General Relativity
This Thesis concerns a thin fluid shell embedded in its own gravitational field. The starting point is a work of
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Anomalous Scaling from Controlled Closure in a Shell Model of Turbulence
We present a model of hydrodynamic turbulence for which the program of computing the scaling exponents from first principles can
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Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?
Recently available near-infrared interferometric data on late-type stars show a strong increase of diameter for asymptotic giant branch (AGB) stars
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A reformulation of the Barrabes-Israel null-shell formalism
We consider a situation in which two metrics are joined at a null hypersurface. It often occurs that the union
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Aspects of on-shell supersymmetry
We study classical field theories that do not admit an action principle, implying that their formulation is entirely in terms
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ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion
The "born-again" PNe V605 Aql (A58) and V4344 Sgr (Sakurai) give us the rare chance to follow shell formation and
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A unified formalism for the core mass-luminosity relations of shell-burning stars
The luminosity evolution of stars with highly condensed cores surrounded by nuclear-burning shell(s) is analytically investigated with the aid of
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Automatic Shell Detection in CGPS Data
A numerical code aiming at the automatic detection of spherical expanding HI shells in radio data-cubes is presented. The following
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A vestige low metallicity gas shell surrounding the radio galaxy 0943-242 at z=2.92
Observations are presented showing the doublet CIV 1550 absorption lines superimposed on the CIV emission in the radio galaxy 0943-242.
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B.R.S. renormalisation of some on-shell closed algebras of symmetry transformations : the example of supersymmetric non-linear sigma models : the N=1 case
In order to study in a regularisation free manner the renormalisability of d=2 supersymmetric non-linear $\si$ models, one has to
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Bursts and Shocks in a Continuum Shell Model
We study a "burst" event, i. e. the evolution of an initial condition having support only in a finite interval
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Casimir energy for self-interacting scalar field in a spherical shell
In this paper we calculate the Casimir energy for spherical shell with massless self-interacting scalar filed which satisfying Dirichlet boundary
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CIV absorption from hot gas inside supergiant shell LMC4 observed with HST and IUE
High resolution ultraviolet spectra with HST-GHRS of two stars in the direction of the supergiant shell LMC4 unambiguously show absorption
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Comment on ``Shell Filling and Spin Effects in a Few Electron Quantum Dot'' [PRL 77, 3613 (1996)]
We briefly report on calculated addition spectra for electrons in a circular quantum dot with perpendicular magnetic field. We compare
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Complete Initial State Radiation to off-Shell $Z^0$~PAIR Production in $e^+e^-$~ANNIHILATION
A cross-section calculation for the Standard Model reaction $e^+e^- \rightarrow (Z^0Z^0) \rightarrow f_1\bar{f_1}f_2\bar{f_2}$ including the effects of the finite $Z^0$~width
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Compton scattering by pion: there is no room for the off-shell effects
We show that the off-shell contributions in Compton scattering by pion may exist only in the single exchange diagrams. These
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Conformally Invariant Off-shell Strings
Recent advances in non-critical string theory allow a unique continuation of critical Polyakov string amplitudes to off-shell momenta, while preserving
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Confronting atomic data with Fe L-shell spectra of stellar coronae
It is common to suggest the uncertainties in the atomic data for explaining difficulties that arise in interpreting astrophysical x-ray
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