Astronomy and astrophysics: A European journal

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  Año 2004, Vol. 426, Número 2

  • A super massive black hole binary in 3C 66B: Future observational perspectives

    F. De Paolis, A. A. Nucita, G. Ingrosso

    págs. 379-386

    

  • Probing turbulence in the Coma galaxy cluster

    P. Schuecker, A. Finoguenov

    págs. 387-398

    

  • On the importance of the few most massive stars: The ionizing cluster of NGC 588

    L. Jamet, M. Cervino, R. M. G. Delgado, G. Stasinska, E. Pérez

    págs. 399-414

    

  • Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27

    J. J. M. i. Zand, F. Frontera, L. Amati

    págs. 415-424

    

  • A dust emission model of Lyman-break galaxies

    T. T. Takeuchi

    págs. 425-436

    

  • Multi-band optical micro-variability observations of the BL Lac object S4 0954+658

    I. E. Papadakis, V. Samaritakis

    págs. 437-444

    

  • The dynamical state of a thick cloudy torus around an AGN

    W. J. Duschl, T. Becker

    págs. 445-454

    

  • Assessing the galaxy population out to z ~ 2 using the Hubble Deep Field South

    T. Wiegert, D. F. de Mello

    págs. 455-462

    

  • The B3-VLA CSS sample. V. VLBA images at 6 and 3.6 cm

    M. Orienti, D. Dallacasa

    págs. 463-470

    

  • Molecular and ionized gas in the tidal tail in Stephan's Quintet

    U. Lisenfeld

    págs. 471-480

    

  • The twin-jet system in NGC 1052: VLBI-scrutiny of the obscuring torus

    M. Kadler

    págs. 481-494

    

  • Initial mass function in the South-Western part of M 31

    P. Nedialkov, T. Veltchev

    págs. 495-502

    

  • A study of high velocity molecular outflows with an up-to-date sample

    M. Zhao, Y. Wei, Y. Wu

    págs. 503-516

    

  • The quest for C~2N in space. A search with the IRAM 30 m telescope towards IRC+10216

    G. W. Fuchs

    págs. 517-522

    

  • The hot core-ultracompact H II connection in G10.47+0.03

    I. Pascucci

    págs. 523-534

    

  • A radio and mid-infrared survey of northern bright-rimmed clouds

    L. K. Morgan, J. S. Urquhart, M. A. Thompson

    págs. 535-546

    

  • Optical and near infrared observations of SN 1998bu

    J. Spyromilio

    págs. 547-554

    

  • Intermediate-velocity gas observed towards the Shajn 147 SNR

    B. Y. Welsh, S. Sallmen

    págs. 555-566

    

  • The supernova remnant G 6.4-0.1 and its environment

    F. Mavromatakis

    págs. 567-576

    

  • The shortest period M dwarf eclipsing system BW3 V38. II. Determination of absolute elements

    J. Montalbán, C. Maceroni

    págs. 577-586

    

  • A study of the low-frequency quasi-periodic oscillations in the X-ray light curves of the black hole candidate XTE J1859+226

    P. Casella, T. Belloni

    págs. 587-600

    

  • VLTI near-IR interferometric observations of Vega-like stars. Radius and age of alphaPsA, betaLeo, betaPic, epsilonEri and tauCet

    A. D. de Souza, P. Kervella, F. Thévenin, V. C. d. Foresto, E. Di Folco

    págs. 601-618

    

  • C, S, Zn and Cu abundances in planet-harbouring stars

    N. C. Santos, G. Israelian, A. Ecuvillon

    págs. 619-630

    

  • The parallax, mass and age of the PSR J2145-0750 binary system

    O. Lohmer, A. Jessner, T. Driebe, M. Kramer

    págs. 631-640

    

  • RR Lyrae variables in Galactic globular clusters. IV. Synthetic HB and RR Lyrae predictions

    S. Cassisi, M. Castellani

    págs. 641-650

    

  • Beryllium in turnoff stars of NGC 6397: Early Galaxy spallation, cosmochronology and cluster formation

    L. Pasquini, P. Bonifacio

    págs. 651-658

    

  • High-energy observations of the state transition of the X-ray nova and black hole candidate XTE J1720-318

    J. Rodriguez, M. C. Bel

    págs. 659-668

    

  • The old nova DQ Her (1934). The eclipse of the triple-peaked H~a~l~p~h~a profile

    E. Mastrantonio, A. Bianchini

    págs. 669-676

    

  • The polarization of drifting subpulses

    R. T. Edwards

    págs. 677-686

    

  • Hydrodynamic models for beta Cephei variables. I. BW Vulpeculae revisited

    E. Chapellier, A. Fokin, P. Mathias

    págs. 687-694