Hydrodynamics Polarization ISM molecules Cosmology Sedimentology Cosmic background radiation Instabilities Delta Galaxies active Mars 2020 Cosmological model Gale crater Sismologie Magnetohydrodynamics MHD Galaxies clusters general Turbulence Planetary systems Accretion disks Methods numerical Stratigraphy Galaxies clusters intracluster medium Black hole physics Satellite Stars low-mass Astrophysics Astrophysics - Solar and Stellar Astrophysics Accretion Magnetic reconnection Star formation Methods statistical Astrophysics - Instrumentation and Methods for Astrophysics Galaxies star formation Galaxies ISM Stars formation ISM clouds Magnetic fields Asteroseismology Epos-France Astrophysics - Earth and Planetary Astrophysics ISM structure Astrophysics - High Energy Astrophysical Phenomena ISM jets and outflows Techniques polarimetric Stars rotation Ionosphere Cosmic background radiation polarization Accretion discs Jezero crater Stars imaging Sensitivity Stars solar-type Stars oscillations Stars interiors Extinction Physics - Space Physics Techniques spectroscopic Observatory Stars evolution Radiative transfer Methods data analysis ISM abundances Dust Catalogs Gamma rays general Galaxies formation Infrared ISM Cosmic rays Stars neutron Stars magnetic field Dark energy X-rays galaxies clusters Plasmas Perseverance Astrochemistry Galaxies high-redshift Seismology Sun magnetic fields X-rays general GLAST Large-scale structure of Universe Galaxy Spectroscopy Methods observational Solar wind Astrophysics - Astrophysics of Galaxies Stars activity MAVEN Cherenkov Telescope Array Dark matter Galaxies evolution X-rays binaries Interstellar medium Waves Cosmological parameters Cosmology observations Surveys Submillimeter ISM Mars Magnetosphere Structure