Astrophysics
Hydrodynamic Interaction between the Be Star and the Pulsar in the TeV Binary PSR B1259-63/LS 2883
Influence of cosmological models on the GZK horizon of ultrahigh energy protons
INTEGRAL and Swift observations of IGRJ19294+1816 in outburst
Jet Formation in the magnetospheres of supermassive black holes: analytic solutions describing energy loss through Blandford-Znajek processes
Lower Bound on the Magnetic Field Strength of a Magnetar from Analysis of SGR Giant Flares
Mass accretion to young stars triggered by flaring activity in circumstellar disks
Mass and radius estimation for the neutron star in X-ray burster 4U 1820-30
Modeling supernova remnants: effects of diffusive cosmic-ray acceleration on the evolution, application to observations
Molecular and Atomic Gas toward HESS J1745-303 in the Galactic Center: Further Support for the Hadronic Scenario
New Optical/UV Counterparts and the Spectral Energy Distributions of Nearby, Thermally Emitting, Isolated Neutron Stars
Non-Fermi liquid behavior of the drag and diffusion coefficients in QED plasma
Observational constraints on the external shock prior emission hypothesis of GRBs
Observations of Lensed Relativistic Jets as a Tool of Constraining Lens Galaxy Parameters
On the nature of the first transient Z-source XTE J1701-462: its accretion disk structure, neutron star magnetic field strength, and hard tail
Photometric Observations of Three High Mass X-Ray Binaries and a Search for Variations Induced by Orbital Motion
Photopolarimetric Monitoring of Blazars in the Optical and Near-Infrared Bands with the Kanata Telescope. I. Correlations between Flux, Color, and Polarization
Population III Gamma-Ray Bursts and Breakout Criteria for Accretion-Powered Jets
Quantum Gravity phenomenology: achievements and challenges
Radiative efficiency and thermal spectrum of accretion onto Schwarzschild black holes
Rest-frame properties of 32 gamma-ray bursts observed by the Fermi Gamma-Ray Burst Monitor
Self-consistent Seeding of the Interchange Instability in Dipolarization Fronts
Some necessary conditions for allowing the PQ scale as high as M_{GUT} in SUSY models with an axino or neutralino LSP