Cosmic ray transport in galaxy clusters: implications for radio halos, gamma-ray signatures, and cool core heating
Astronomy & Astrophysics EDP Sciences 527 (2011) a99
EVOLUTION OF SHOCKS AND TURBULENCE IN MAJOR CLUSTER MERGERS
The Astrophysical Journal American Astronomical Society 726:1 (2011) 17
Resistive Generation of Intergalactic Magnetic Field at Cosmic Dawn
NUMERICAL MODELING OF SPACE PLASMA FLOWS: ASTRONUM-2011 459 (2011) 125-+
A hybrid scheme for gas–dust systems stiffly coupled via viscous drag
Journal of Computational Physics Elsevier 229:10 (2010) 3916-3937
Mg ii ABSORPTION SYSTEMS WITH W0 ⩾ 0.1 Å FOR A RADIO SELECTED SAMPLE OF 77 QUASI-STELLAR OBJECTS AND THEIR ASSOCIATED MAGNETIC FIELDS AT HIGH REDSHIFT**Based on observations made with ESO telescopes at the Paranal Observatory under Programme IDs 075.A-0841 and 076.A-0860.
The Astrophysical Journal American Astronomical Society 711:1 (2010) 380-388