Astronomy and astrophysics: A European journal

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  Año 2006, Vol. 453, Número 1

  • Simulated synchrotron emission from pulsar wind nebulae

    L. Del Zanna

    págs. 621-634

    

  • Modelling the Galactic interstellar extinction distribution in three dimensions

    D. J. Marshall

    págs. 635-652

    

  • The production of short-lived radionuclides by new non-rotating and rotating Wolf-Rayet model stars

    S. Goriely, M. Arnould

    págs. 653-660

    

  • Non-spherical core collapse supernovae. II. The late-time evolution of globally anisotropic neutrino-driven explosions and their implications for SN 1987 A

    K. Kifonidis

    págs. 661-678

    

  • The topology and polarisation of subbeams associated with the "drifting" subpulse emission of pulsar B0943+10. IV. Q-to-B-mode recovery dynamics

    S. A. Suleymanova, J. M. Rankin

    págs. 679-686

    

  • The stability of toroidal fields in stars

    J. Braine

    págs. 687-698

    

  • The diagnosis of the mean quadratic magnetic field of Ap stars

    S. Hubrig, G. Mathys

    págs. 699-716

    

  • Lithium abundances for early F stars: new observational constraints for the Li dilution

    G. Jasniewicz, A. Recio-Blanco

    págs. 717-722

    

  • (RN) NLTE analysis of the solar potassium abundance

    H. W. Zhang

    págs. 723-728

    

  • Solar bursts gyrosynchrotron emission from three-dimensional sources

    P. J. A. Simoes, J. E. R. Costa

    págs. 729-736

    

  • (RN) Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Demoulin equilibrium

    T. Wiegelmann

    págs. 737-742

    

  • Cross-identifications and astro-photometric comparisons of the ICRF with recent catalogs of quasars

    J. Souchay, A. M. Gontier

    págs. 743-750

    

  • Stark parameters of neutral helium 318.8 nm line

    R. J. Pelaez, V. R. Gonzalez

    págs. 751-754

    

  • Nuclear spin conversion of formaldehyde in protostar environments induced by non reactive collisions

    M. Tudorie, P. Cacciani

    págs. 755-760

    

  • An analysis method for time ordered data processing of dark matter experiments

    E. Moulin, J.F. Macías-Pérez

    págs. 761-768

    

  • New grids of stellar models including tidal-evolution constants up to carbon burning. III. From 0.8 to 125 M: the Large Magellanic Cloud (Z = 0.007-0.01)

    A. Claret

    págs. 769-771