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