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