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  • Cambridge University Press (CUP)  (4)
Materialart
Verlag/Herausgeber
  • Cambridge University Press (CUP)  (4)
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  • 1
    Online-Ressource
    Online-Ressource
    Cambridge University Press (CUP) ; 1987
    In:  Symposium - International Astronomical Union Vol. 117 ( 1987), p. 279-279
    In: Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 117 ( 1987), p. 279-279
    Kurzfassung: When one builds a code to simulate numerically a process, the first concern is the range of validity of the results. This can be accessed empirically, though the results can be misleading if the tests are too naive. For particle-mesh codes simulating the gravitational clustering, an analytical theory has been proposed in Bouchet et al. 1985. It yields the numerical dispersion relation of the system in the linear regime, and thus describes how the linear growth rate is affected by the discretisation. The theoretical predictions are in agreement with the results of actual numerical experiments: both show that the results of standart particle-mesh codes should not be trusted at distances smaller than 6 to 8 grid-spacing Δx (depending on the detail of the algorithm).
    Materialart: Online-Ressource
    ISSN: 0074-1809
    Sprache: Englisch
    Verlag: Cambridge University Press (CUP)
    Publikationsdatum: 1987
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    Cambridge University Press (CUP) ; 1994
    In:  Symposium - International Astronomical Union Vol. 159 ( 1994), p. 319-319
    In: Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 159 ( 1994), p. 319-319
    Kurzfassung: We present ground-based data of the BL Lac object PKS 2155-305 obtained during a large international campaign spanning the electro–magnetic spectrum from the radio waves to X-rays in November 1991. For the complete description of the observations and data analysis we refer to the paper by Courvoisier et al. 1993, and references therein. The ground-based data include radio, infrared JHKL and UBVRI fluxes as well as optical and near IR polarimetry. The broad-band optical and near IR data from U to I exhibit the same behaviour in all bands: the flux nearly doubled over the well-covered period of 23 days. The cross-correlation function does not reveal any significant changes in the light-curves. Though significant variations in 24 hours have been recorded, the cumulated Fourier power spectrum drops to the noise level for periods shorter than 2.5 days. The spectral index remained constant. The polarised flux varied by a larger factor than the total flux and did not follow the same pattern. The degree of polarisation and polarisation angle are nearly independent of the wavelength and are strongly correlated in all filters. In the radio domain the spectral index increased from −0.1 on November 5 to +0.02 on 25-th. The absence of the lag between the optical and infrared bands and the polarisation variations are consistent with a model in which the variability is caused by micro-lensing of the source (Stickel, Fried and Kühr 1988). One would, however, expect in this model that the variation in the polarisation and the total flux are tightly correlated contrary to what is observed. The constant shape of the continuum spectral energy suggests that only the number of electrons whose emission is beamed towards the observer changes, rather than the arrival of fresh electrons that are being accelerated. The variability of the polarisation may be explained by changes in the geometry of the magnetic field (dominant direction). This is consistent with the observed variations of the polarisation angle.
    Materialart: Online-Ressource
    ISSN: 0074-1809
    Sprache: Englisch
    Verlag: Cambridge University Press (CUP)
    Publikationsdatum: 1994
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 3
    Online-Ressource
    Online-Ressource
    Cambridge University Press (CUP) ; 1994
    In:  Symposium - International Astronomical Union Vol. 159 ( 1994), p. 63-72
    In: Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 159 ( 1994), p. 63-72
    Kurzfassung: Brief review of AGNs observations in the X-ray / soft gamma-ray bands with the orbital observatory GRANAT is presented. For three well known bright objects (3C273, NGC4151 and Cen A) broad band (3 keV–few hundreds keV) spectra have been obtained. Imaging capabilities allowed accurate (several arcminutes) identification of these objects with sources of hard X-rays. The spectrum of NGC4151 above ≈ 50 keV was found to be much steeper than that in most of the previous observations, while in standard X-ray band the spectrum agrees with observed previously. The comparison of the observed spectra with that of the X-Ray Background (XRB) indicates that sources similar to NGC4151 could reproduce the shape of XRB spectrum in 3–60 keV band. Cen A was observed in the very low state during most of observations in 1990–1993, except for two observations in 1991. The variability of the hard X-ray flux has been detected on the time scales of several days.
    Materialart: Online-Ressource
    ISSN: 0074-1809
    Sprache: Englisch
    Verlag: Cambridge University Press (CUP)
    Publikationsdatum: 1994
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 4
    Online-Ressource
    Online-Ressource
    Cambridge University Press (CUP) ; 1981
    In:  Proceedings, annual meeting, Electron Microscopy Society of America Vol. 39 ( 1981-08), p. 354-355
    In: Proceedings, annual meeting, Electron Microscopy Society of America, Cambridge University Press (CUP), Vol. 39 ( 1981-08), p. 354-355
    Kurzfassung: Convergent beam electron diffraction is a powerful technique for determining the crystal structure of a material in TEM. In this paper we have applied it to the study of the intermetallic phases in the Cu-rich end of the Cu-Zr system. These phases are highly ordered. Their composition and structure has been previously studied by microprobe and x-ray diffraction with sometimes conflicting results. The crystalline phases were obtained by annealing amorphous sputter-deposited Cu-Zr. Specimens were thinned for TEM by ion milling and observed in a Philips EM 400. Due to the large unit cells involved, a small convergence angle of diffraction was used; however, the three-dimensional lattice and symmetry information of convergent beam microdiffraction patterns is still present. The results are as follows: 1) 21 at% Zr in Cu: annealed at 500°C for 5 hours. An intermetallic phase, Cu3.6Zr (21.7% Zr), space group P6/m has been proposed near this composition (2). The major phase of our annealed material was hexagonal with a point group determined as 6/m.
    Materialart: Online-Ressource
    ISSN: 0424-8201 , 2690-1315
    Sprache: Englisch
    Verlag: Cambridge University Press (CUP)
    Publikationsdatum: 1981
    SSG: 11
    Standort Signatur Einschränkungen Verfügbarkeit
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