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21cm line AGN AGN feedback AGN jets ALMA Andromeda B-mode polarization CGM CIB CMB CMZ DLA DM Halo Faraday rotation First star G2 GMC GPU GRB Gaia Galactic center Godunov scheme HPC HST Hydra A IGM IR JSPS James Webb James Webb telescope LAE LOFAR Lyman Alpha Blobs Lyman Alpha Forest M-sigma relation M33 MHD MRI Milky Way N-body simulation N-body simulations NLS1 Nobeyama 45m radio telescope PopIII stars Riemann solvers SKA SMBH SMBH binaries SMBH mergers SOLAR-C SPH Sgr* SgrA* Solar Corona Subaru TDDFT TMT UHECR ULIRG Vlasov-Poisson simulations WHIM X-rays X線偏光 X線天体物理 absorption system accretion accretion discs alma amino acids astrometry awards barred galaxy black holes chemodynamics clouds collisionless systems computational fluid dynamics coronagraphs cosmic magnetic fields cosmic rays cosmological simulations cosmology dark matter dust dusty torus dwarf galaxies dynamical friction early type galaxies early universe exoplanets first galaxies first stars galactic disk galactic halos galaxy clusters galaxy evolution galaxy formation galaxy fromation galaxy interactions galaxy mergers general relativity globular clusters gravitational waves high-energy astrophysics high-z galaxies hydrodyanmics hydrodynamics inflation intergalactic magnetic fields interstellar molecules large scale structure leisure m-sigma relation machine learning masers massive stars molecular clouds molecular cores molecular gas morphology-density relation neutrinos numerical simulation numerical simulations observation observations outreach particle acceleration physical constants planet formation polarization protocluster protoclusters protoplanetary discs protostars protostellar disc protostellar discs pulsars quasars radiation hydrodynamics radiative feedback radiative transfer radio galaxies radio observation radio observations reionization relativistic jets self-gravitating systems semi-analytic models seyfert galaxies solar wind star formation starbursts stellar populations structure formation submm submm galaxies supernova supernova remnants supernovae transients turbulence visualization

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21cm line AGN AGN feedback AGN jets ALMA Andromeda B-mode polarization CGM CIB CMB CMZ DLA DM Halo Faraday rotation First star G2 GMC GPU GRB Gaia Galactic center Godunov scheme HPC HST Hydra A IGM IR JSPS James Webb James Webb telescope LAE LOFAR Lyman Alpha Blobs Lyman Alpha Forest M-sigma relation M33 MHD MRI Milky Way N-body simulation N-body simulations NLS1 Nobeyama 45m radio telescope PopIII stars Riemann solvers SKA SMBH SMBH binaries SMBH mergers SOLAR-C SPH Sgr* SgrA* Solar Corona Subaru TDDFT TMT UHECR ULIRG Vlasov-Poisson simulations WHIM X-rays X線偏光 X線天体物理 absorption system accretion accretion discs alma amino acids astrometry awards barred galaxy black holes chemodynamics clouds collisionless systems computational fluid dynamics coronagraphs cosmic magnetic fields cosmic rays cosmological simulations cosmology dark matter dust dusty torus dwarf galaxies dynamical friction early type galaxies early universe exoplanets first galaxies first stars galactic disk galactic halos galaxy clusters galaxy evolution galaxy formation galaxy fromation galaxy interactions galaxy mergers general relativity globular clusters gravitational waves high-energy astrophysics high-z galaxies hydrodyanmics hydrodynamics inflation intergalactic magnetic fields interstellar molecules large scale structure leisure m-sigma relation machine learning masers massive stars molecular clouds molecular cores molecular gas morphology-density relation neutrinos numerical simulation numerical simulations observation observations outreach particle acceleration physical constants planet formation polarization protocluster protoclusters protoplanetary discs protostars protostellar disc protostellar discs pulsars quasars radiation hydrodynamics radiative feedback radiative transfer radio galaxies radio observation radio observations reionization relativistic jets self-gravitating systems semi-analytic models seyfert galaxies solar wind star formation starbursts stellar populations structure formation submm submm galaxies supernova supernova remnants supernovae transients turbulence visualization

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Recent Posts

Formation of Astrophysical Objects 2024

Oct 18, 2024

Star formation induced by cloud-cloud collisions in nearby barred galaxies

Sep 17, 2024

Formation of intermediate-mass black hole in forming star clusters

Jul 16, 2024

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