Astronomy and astrophysics: A European journal

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  Año 2005, Vol. 433, Número 1

  • Thermal condensation in a turbulent atomic hydrogen flow

    P. Hennebelle, E. Audit

    págs. 1-14

    

  • Erratum: "Swing Absorption" of fast magnetosonic waves in inhomogeneous media

    B. M. Shergelashvili

    págs. 15-16

    

  • Thermodynamic evolution of the cosmological baryonic gas. II. Galaxy formation

    J.-M. Alimi

    págs. 17-30

    

  • Structure of visible and dark matter components in spiral galaxies at redshifts z = 0.5-0.9

    A. Tamm, P. Tenjes

    págs. 31-42

    

  • A wide-field photometric study of the globular cluster system of NGC 4636

    B. Dirsch, Y. Schuberth

    págs. 43-56

    

  • A family of models of partially relaxed stellar systems. II. Comparison with the products of collisionless collapse

    T. S. van Albada, M. Trenti, G. Bertin

    págs. 57-72

    

  • Evidence of intense hot (340 K) dust emission in 3CR radio galaxies. The most dissipative source of cooling in AGNs

    B. Rocca-Volmerange

    págs. 73-78

    

  • Asymmetrical structure of ionization and kinematics in the Seyfert galaxy NGC 5033

    E. Mediavilla

    págs. 79-86

    

  • On the X-ray emission of z ~ 2 radio galaxies: IC scattering of the CMB and no evidence for fully-formed potential wells

    R. A. Overzier

    págs. 87-100

    

  • Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton

    R. Piffaretti

    págs. 101-112

    

  • GRB 040403: A faint X-ray rich gamma-ray burst discovered by INTEGRAL

    S. Mereghetti

    págs. 113-116

    

  • L- and M-band imaging observations of the Galactic Center region

    T. Viehmann

    págs. 117-126

    

  • An estimate of the time variation of the abundance gradient from planetary nebulae. II. Comparison with open clusters, cepheids and young objects

    W. J. Maciel

    págs. 127-136

    

  • Binary formation within globular clusters: X-ray clues

    B. Gendre

    págs. 137-142

    

  • Probing the nature of possible open cluster remnants with the Southern Proper Motion Program

    D. I. Dinescu, G. Carraro

    págs. 143-150

    

  • Identification of a complete sample of northern ROSAT All-Sky Survey X-ray sources. VIII. The late-type stellar component

    F.-J. Zickgraf

    págs. 151-172

    

  • The thick disc component of the Galaxy from near infrared colour-magnitude diagrams

    A. Cabrera-Lavers

    págs. 173-184

    

  • alpha-, r-, and s-process element trends in the Galactic thin and thick disks

    T. Bensby, I. Lundstrom, S. Feltzing

    págs. 185-204

    

  • High spatial resolution radio continuum observations of compact H II regions in the Magellanic Clouds

    N. L. Martín-Hernández

    págs. 205-216

    

  • Shock-induced PDR in the Herbig-Haro object HH 2

    J. Cernicharo, B. Lefloch

    págs. 217-228

    

  • Magnetic field amplification in Tycho and other shell-type supernova remnants

    E. G. Berezhko, H. J. Volk, L. T. Ksenofontov

    págs. 229-240

    

  • A search for interstellar absorptions towards Sgr dSph

    S. Monai, P. Bonifacio

    págs. 241-246

    

  • Models of accreting gas giant protoplanets in protostellar disks

    J. C. B. Papaloizou

    págs. 247-266

    

  • Pulsation of the K 2.5 giant star GSC 09137-03505?

    T. Kallinger

    págs. 267-274

    

  • Thermal radiation from magnetic neutron star surfaces

    J. F. Pérez-Azorín

    págs. 275-284

    

  • Abundance correlations in mildly metal-poor stars. II. Light elements (C to Ca)

    H. Decauwer

    págs. 285-296

    

  • Photometric periods of HN Peg from multichannel analysis

    J. You, R. Duemmler

    págs. 297-304

    

  • Aldebaran's angular diameter: How well do we know it?

    A. Richichi, V. Roccatagliata

    págs. 305-312

    

  • A layered model for non-thermal radio emission from single O stars

    M. C. Runacres, S. van Loo

    págs. 313-322

    

  • A simple model for the saturation of coronal X-ray emission of rapidly rotating late-type stars

    R. D. Ryan, T. Neukirch

    págs. 323-334