Population Synthesis of Radio and Gamma-ray Pulsars in the Fermi Era

Population Synthesis of Radio Pulsars in the Fermi Era

Population synthesis studies of isolated neutron stars with magnetic field decay

Positron annihilation as a cosmic-ray probe

Positron Annihilation on Polycyclic Aromatic Hydrocarbon molecules in the Interstellar Medium

Positron annihilation spectrum from the Galactic Centre region observed by SPI/INTEGRAL, revisited: annihilation in a cooling ISM?

Positron transport in the interstellar medium

Positrons from cosmic rays interactions and dark matter annihilations

Positrons from pulsar winds

Possibility of conversion of neutron star to quark star in presence of high magnetic field

Possible Charge-Exchange X-Ray Emission in the Cygnus Loop Detected with Suzaku

Possible Distance Indicators in Gamma-ray Pulsars

Possible gamma-ray emission of radio intermediate AGN III Zw 2 and its implication on the evolution of jets in AGNs

Possible Interpretations of the High Energy Cosmic Ray Electron Spectrum measured with the Fermi Space Telescope

Possible Origin of Rapid Variability of Gamma-Ray Bursts due to Convective Energy Transfer in Hyperaccretion Disks

Possible origin of viscosity in the Keplerian accretion disks due to secondary perturbation: Turbulent transport without magnetic field

Possible Origins of Dispersion of the Peak Energy--Brightness Correlations of Gamma-Ray Bursts

Possible Resonances in the 12C + 12C Fusion Rate and Superburst Ignition

Possible structure in the cosmic ray electron spectrum measured by the ATIC-2 and ATIC-4 experiments

Possible twin kHz Quasi Periodic Oscillations in the accreting millisecond X-ray Pulsar IGR J17511-3057