págs. 333-340
págs. 341-352
XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87
J. S. Kaastra, N. Werner, H. Bohringer
págs. 353-360
Galaxy pairs in cosmological simulations: effects of interactions on colours and chemical abundances
P. B. Tissera, C. Scannapieco, M. J. Perez
págs. 361-370
(RN) Downsizing of star-forming galaxies by gravitational processes
Y. Taniguchi, H. Mouri
págs. 371-374
págs. 375-390
Dynamics of the NGC 4636 globular cluster system. An extremely dark matter dominated galaxy?
Y. Schuberth, T. Richtler
págs. 391-406
págs. 407-414
Discovery of a cluster of galaxies behind the Milky Way: X-ray and optical observations
R. L. de Oliveira
págs. 415-422
págs. 423-440
págs. 441-452
págs. 453-464
The CFHTLS real time analysis system: "optically selected GRB afterglows". Overview and performance
J.-L. Atteia, F. Malacrino
págs. 465-476
págs. 477-488
Search and analysis of blue straggler stars in open clusters
F. De Angeli, F. De Marchi
págs. 489-498
Deep near-IR photometry of eight metal-poor globular clusters in the Galactic bulge and halo
J.-W. Kim
págs. 499-510
On the age of the TW Hydrae association and 2M1207334-393254
D. B. y Navascues
págs. 511-518
Radio emission from shell-type supernova remnants
A. I. Asvarov
págs. 519-534
págs. 535-544
C2D Spitzer-IRS spectra of disks around T Tauri stars. II. PAH emission features
V. C. Geers, J. C. Augereau, K. M. Pontoppidan
págs. 545-556
The rapidly pulsating subdwarf B star PG 1325+101. I. Oscillation modes from multisite observations
S. Bernabei, G. Fontaine, A. Bonanno, S. Charpinet, R. Silvotti
págs. 557-564
The rapidly pulsating subdwarf B star PG 1325+101. II. Structural parameters from asteroseismology
S. Charpinet, R. Silvotti
págs. 565-576
The Blazhko effect of RR Lyrae in 2003-2004
H. A. Smith, K. D. Gazeas, K. Kolenberg
págs. 577-588
págs. 589-596
Erratum: The bright spiky emission of pulsar B0656+14
G. A. E. Wright, P. Weltevrede
págs. 597-598
págs. 599-612
págs. 613-626
págs. 627-640
págs. 641-650
Study of an extended EUV filament using SoHO/SUMER observations of the hydrogen Lyman lines
B. Schmieder, P. Heinzel, P. Schwartz
págs. 651-662
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