Astronomy and astrophysics: A European journal

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  Año 2004, Vol. 424, Número 2

  • A model for quasi-spherical magnetized accretion flow

    M. Shadmehri

    págs. 379-388

    

  • Superposition of blackbodies and the dipole anisotropy: A possibility to calibrate CMB experiments

    J. Chluba, R. A. Sunyaev

    págs. 389-408

    

  • Radio source contamination of the Sunyaev-Zeldovich effect in galaxy clusters

    M. Massardi, G. De Zotti

    págs. 409-414

    

  • Dark energy versus Omega~m = 1 in the growth of matter perturbations

    M. Membrado, J. A. L. Aguerri

    págs. 415-428

    

  • Magnetic fields and Faraday rotation in clusters of galaxies

    M. Murgia, F. Govoni, L. Feretti, G. Giovannini

    págs. 429-446

    

  • Ionized gas and stellar kinematics of seventeen nearby spiral galaxies

    J. C. V. Beltrán, A. Pizzella, E. M. Corsini

    págs. 447-454

    

  • On-axis spectroscopy of the z = 0.144 radio-loud quasar HE 1434-1600: an elliptical host with a highly ionized ISM

    F. Courbin, G. Letawe

    págs. 455-464

    

  • The radial extinction profiles of late-type galaxies

    Emanuele Boselli, S. Boissier

    págs. 465-476

    

  • The very early afterglow powered by ultra-relativistic mildly magnetized outflows

    Y. Z. Fan, D. M. Wei, C. F. Wang

    págs. 477-484

    

  • Kinematics of the ionised gas in the spiral galaxy NGC 2403

    F. Fraternali, T. Oosterbroek

    págs. 485-496

    

  • The WEBT campaigns on BL Lacertae. Time and cross-correlation analysis of optical and radio light curves 1968-2003

    C. M. Raiteri, M. Villata

    págs. 497-508

    

  • Kinematics of two dwarf galaxies in the NGC 6946 group

    A. Begum, J. N. Chengalur

    págs. 509-518

    

  • Naked active galactic nuclei

    M. R. S. Hawkins

    págs. 519-530

    

  • The ISOPHOT-MAMBO survey of 3CR radio sources: Further evidence for the unified schemes

    S. A. H. Muller, M. Haas

    págs. 531-544

    

  • Discovery of optically faint obscured quasars with Virtual Observatory tools

    P. Padovani, M. G. Allen

    págs. 545-560

    

  • Mg II spectral line broadening in helium, oxygen and argon-helium plasmas

    S. Djenize, A. Sreckovic, S. Bukvic

    págs. 561-564

    

  • Seed fields for galactic dynamos by the magnetorotational instability

    L. L. Kitchatinov

    págs. 565-570

    

  • First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops

    A. Benoit

    págs. 571-582

    

  • The kinematics of the bi-lobal supernova remnant G 65.3+5.7. II

    J. Meaburn, J. A. López, P. Boumis, F. Mavromatakis

    págs. 583-588

    

  • Imaging chemical differentiation around the low-mass protostar L483-mm

    J. K. Jorgensen

    págs. 589-602

    

  • Accretion in brown dwarfs: An infrared view

    A. Natta, J. Muzerolle, L. Testi

    págs. 603-612

    

  • A search for circumstellar dust disks with ADONIS

    H. Bohnhardt, O. Schutz

    págs. 613-618

    

  • X-ray detections of two young bona-fide brown dwarfs

    H. Bouy

    págs. 619-626

    

  • On the nature of the bimodal initial velocity distribution of neutron stars

    I. Bombaci, S. B. Popov

    págs. 627-634

    

  • The isolated neutron star X-ray pulsars RX J0420.0-5022 and RX J0806.4-4123: New X-ray and optical observations

    C. Motch, F. Haberl, V. E. Zavlin

    págs. 635-646

    

  • Time-resolved photometry and spectroscopy of the new deeply-eclipsing SW Sextantis star HS 0728+6738

    P. Rodriguez-Gil

    págs. 647-656

    

  • Identification of a DO white dwarf and a PG 1159 star in the ESO SN Ia progenitor survey (SPY)

    T. Rauch, K. Werner, N. Christlieb, R. Napiwotzki

    págs. 657-664

    

  • Do weak magnetic fields prevent hydrogen from accreting onto metal-line white dwarf stars?

    S. Friedrich

    págs. 665-670

    

  • Propagating waves in the sunspot umbra chromosphere

    D. V. Makarchik, N. I. Kobanov

    págs. 671-676

    

  • The Sun as an X-ray star: Active region evolution, rotational modulation, and implications for stellar X-ray variability

    S. Orlando

    págs. 677-690