Pulsar Supernovae general Stars formation Galaxies structure Techniques photometric Methods statistical Black hole physics Stars massive Infrared ISM Gravitation Magnetohydrodynamics MHD Galaxies clusters general Surveys Stars interiors ISM structure ISM supernova remnants Galaxies dwarf X-rays galaxies clusters Supernova Stars protostars Observatory ISM general Cosmological parameters Gravitational waves Galaxies evolution Galaxies interactions Gravitational lensing weak Stars oscillations Gamma ray Galaxies jets Cosmic rays Protoplanetary disks Radiation mechanisms non-thermal Waves ISM jets and outflows ISM clouds Astrophysics - Astrophysics of Galaxies Galaxies clusters intracluster medium Stars rotation GLAST Extinction Shock waves Cosmic background radiation Methods data analysis Gamma-ray burst general Dark energy X-rays general HII regions Astrophysics Accretion Asteroseismology Radio continuum galaxies Dust Structure X-rays binaries ISM kinematics and dynamics Cosmology observations Galaxies star formation Binaries general Cosmological model Infrared stars Galaxies high-redshift Magellanic Clouds Gamma ray emission Turbulence Spectral ISM molecules Accretion disks Galaxy Galaxy Astrophysics Radiative transfer Stars evolution Infrared galaxies Pulsars general MHD Large-scale structure of Universe Polarization Stars neutron Cosmology Dark matter Techniques image processing Accretion discs Galaxies active Instabilities Catalogs Hydrodynamics Gamma rays general Acceleration of particles Methods numerical Sensitivity Cherenkov Telescope Array Galaxies ISM Methods observational Gamma rays galaxies Gamma ray burst Galaxies photometry Galaxies starburst Submillimeter galaxies Submillimeter ISM Galaxies formation