Astronomy and astrophysics: A European journal

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  Año 2003, Vol. 411, Número 2

  • Twofold effect of Alfven waves on the transverse gravitational instability

    A. Gazol, T. Passot

    págs. 1-8

    

  • Semi-analytical homologous solutions of the gravo-magnetic contraction

    P. Hennebelle

    págs. 9-20

    

  • XMM-Newton observation of the interacting cluster Abell 3528

    F. Gastaldello

    págs. 21-32

    

  • Approximate angular diameter distance in a locally inhomogeneous universe with nonzero cosmological constant

    A. A. Marino, R. de Ritis, M. Demianski, E. Piconcelli

    págs. 33-40

    

  • An X-ray halo in the "hot-spot" galaxy NGC 2903

    D. Tschoke, G. Hensler

    págs. 41-54

    

  • NIR surface photometry of a sample of nearby spiral galaxies

    N. Castro-Rodríguez

    págs. 55-62

    

  • XMM-Newton observation of the ULIRG NGC 6240. The physical nature of the complex Fe K line emission

    T. Boller

    págs. 63-70

    

  • Ratio of energies radiated in the universe through accretive processes and nucleosynthesis

    J. A. Z. Heras

    págs. 71-76

    

  • (RN) BeppoSAX observations of Seyfert 1s in the Piccinotti sample. I. poorly studied sources

    A. Quadrelli

    págs. 77-82

    

  • (RN) Discovery of new Milky Way star cluster candidates in the 2MASS Point Source Catalog. II. Physical properties of the star cluster CC 01

    J. Borissova

    págs. 83-90

    

  • (RN) How do binary separations depend on cloud initial conditions?

    M. F. Sterzik, R. H. Durisen

    págs. 91-98

    

  • Systematic bias in interstellar magnetic field estimates

    R. Wielebinski, A. Shukurov, D. Sokoloff, R. Beck

    págs. 99-108

    

  • High resolution 21 cm mapping of the Ursa Major Galactic cirrus: Power spectra of the high-latitude HI gas

    M.-A. Miville-Deschênes

    págs. 109-122

    

  • "Thermal" SiO radio line emission towards M-type AGB stars: A probe of circumstellar dust formation and dynamics

    D. G. Delgado

    págs. 123-148

    

  • On the intrinsic shape of molecular clouds

    C. E. Jones, C. M. Brunt, C. R. Kerton

    págs. 149-156

    

  • (RN) First NACO observations of the Brown Dwarf LHS 2397aB

    W. Brandner, E. Masciadri

    págs. 157-160

    

  • Ground-based photometry of the contact binary V1128 Tauri

    G. Tas, O. Cakirli, C. Ibanoglu, S. Evren

    págs. 161-166

    

  • Stellar and circumstellar activity of the Be star omega CMa. II. Periodic line-profile variability

    S. Stefl, T. Rivinius, D. Baade

    págs. 167-180

    

  • Stellar and circumstellar activity of the Be star omega CMa. III. Multiline non-radial pulsation modeling

    M. Maintz, T. Rivinius

    págs. 181-192

    

  • The LBV nature of Romano's star (GR 290) in M 33

    V. F. Polcaro

    págs. 193-196

    

  • Two new bright Ae stars

    S. N. Fabrika, G. A. Wade, D. N. Monin

    págs. 197-202

    

  • Cross-field charge transport by the diocotron instability in pulsar magnetospheres with gaps

    S. Bonazzola, J. Petri, J. Heyvaerts

    págs. 203-214

    

  • The ratio of small to large separations of acoustic oscillations as a diagnostic of the interior of solar-like stars

    I. W. Roxburgh, S. V. Vorontsov

    págs. 215-220

    

  • On the accuracy of the ALI method for solving the radiative transfer equation

    L. Chevallier

    págs. 221-228

    

  • Non-radially pulsating Be stars

    T. Rivinius

    págs. 229-248

    

  • Spatial and temporal fluctuations in sunspots derived from MDI data

    S. K. Solanki

    págs. 249-256

    

  • On the heat transport in a sunspot penumbra

    R. Schlichenmaier

    págs. 257-262

    

  • On the origin of microwave type U-bursts

    A. T. Altyntsev, A. A. Kuznetsov, N. S. Meshalkina

    págs. 263-272

    

  • A study of the causal relationship between the emergence of a twisted magnetic flux rope and a small Halpha two-ribbon flare

    D. H. Brooks, K. Yoshimura, H. Kurokawa

    págs. 273-290

    

  • Evolution of Mercury-like orbits: A numerical study

    O. Karlsson, J. Warell

    págs. 291-308