Astronomy and astrophysics: A European journal

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  Año 2004, Vol. 423, Número 2

  • The MHD Alfven wave oscillation model of kHz Quasi Periodic Oscillations of Accreting X-ray binaries

    C. Zhang

    págs. 401-404

    

  • Cosmic rays from Galactic pulsars

    W. Bednarek, M. Bartosik

    págs. 405-414

    

  • Evidence for TeV gamma ray emission from TeV J2032+4130 in Whipple archival data

    M. J. Lang, D. A. Carter-Lewis

    págs. 415-420

    

  • Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraints

    Z.-H. Zhu

    págs. 421-426

    

  • Chemical abundances in spiral and irregular galaxies. O and N abundances derived from global emission-line spectra

    L. S. Pilyugin

    págs. 427-440

    

  • Starburst activity in the host galaxy of the z = 2.58 quasar J1409+5628

    A. Beelen

    págs. 441-448

    

  • RASS-SDSS Galaxy clusters survey. I. The catalog and the correlation of X-ray and optical properties

    P. Popesso, J. Brinkmann, H. Bohringer

    págs. 449-468

    

  • Statistical properties of local active galactic nuclei inferred from the RXTE 3-20 keV all-sky survey

    M. G. Revnivtsev, S. Y. Sazonov

    págs. 469-480

    

  • The nuclear ring in the unbarred galaxy NGC 278: Result of a minor merger?

    W. J. G. de Blok, L. F. Whyte, J. H. Knapen, J. M. van der Hulst

    págs. 481-494

    

  • X-ray polarization properties of the accretion column in magnetic CVs

    G. Matt

    págs. 495-500

    

  • Ellipsoidal mass models with varying axial ratios

    D. K. Chakraborty

    págs. 501-506

    

  • The metal content of the bulge globular cluster NGC 6528

    B. Barbuy, M. Zoccali

    págs. 507-516

    

  • Chemical enrichment and star formation in the Milky Way disk. III. Chemodynamical constraints

    H. J. Rocha-Pinto

    págs. 517-536

    

  • Mid-infrared sizes of circumstellar disks around Herbig Ae/Be stars measured with MIDI on the VLTI

    R. van Boekel, C. Leinert, L. B. F. M. Waters

    págs. 537-548

    

  • Organic matter in Seyfert 2 nuclei: Comparison with our Galactic center lines of sight

    E. Dartois

    págs. 549-558

    

  • Evolution of irradiated circumbinary disks

    R. Gunther, C. Schafer

    págs. 559-566

    

  • Multi-wavelength analysis of the dust emission in the Small Magellanic Cloud

    C. Bot, F. Bouchy

    págs. 567-578

    

  • Origin of diffuse C II 158 micron and Si II 35 micron emission in the Carina nebula

    M. Mizutani

    págs. 579-592

    

  • Abundances of Planetary Nebulae IC 418, IC 2165 and NGC 5882

    S. R. Pottasch, J. Bernard-Salas

    págs. 593-606

    

  • A study of the EB-type eclipsing binary GR Tauri with mass transfer

    Y.-k. Choy, S.-h. Gu, P.-s. Chen, K.-c. Leung, W.-k. Chung

    págs. 607-612

    

  • Doppler imaging of stellar non-radial pulsations. I. Techniques and numerical experiments

    O. Kochukhov

    págs. 613-628

    

  • A search for shock-excited molecular hydrogen knots in Chamaeleon I very low mass YSOs

    M. Gómez, P. Persi, A. R. Marenzi

    págs. 629-642

    

  • Magellanic Cloud Cepheids: Pulsational and evolutionary modelling vs. observations

    J. R. Buchler

    págs. 643-650

    

  • Serpens X-1 observed by INTEGRAL

    L. Foschini, N. Masetti

    págs. 651-656

    

  • Dust in brown dwarfs. IV. Dust formation and driven turbulence on mesoscopic scales

    C. Helling

    págs. 657-676

    

  • On the determination of oxygen abundances in chromospherically active stars

    T. Morel, G. Micela

    págs. 677-682

    

  • Sodium abundances in nearby disk stars

    T. Gehren, J. R. Shi

    págs. 683-692

    

  • 3D hydrodynamical simulations of corotating interaction regions in rotating line-driven stellar winds

    L. Dessart

    págs. 693-704

    

  • The spectroscopic signature of roAp stars

    T. Ryabchikova

    págs. 705-716

    

  • Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption?

    D. Ruzdjak, B. Vrsnak

    págs. 717-728