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University of Tsukuba, Center for Computational Sciences

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Tsukuba Uchu Forum

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Uchu Forum
Tsukuba Uchu Forum...

About the Uchu Forum

The Tsukuba Uchu-Forum are a series of talks, which universities and research institutes in the Tsukuba area participate in. It is an event unique to the Kenkyugakuen-toshi.

Usual place and time:

Every third Tuesday of the month
13:30 ~ 15:00
Center for Computational Sciences, University of Tsukuba, Workshop Room or Seminar room.

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21cm line AGN AGN feedback AGN jets ALMA Andromeda Astrochemistry B-mode polarization CGM CIB CMB CMZ DLA DM Halo Faraday rotation First star G2 GMC GPU GRB Gaia Galactic Archeology Galactic center Godunov scheme HPC HST Hydra A IGM IMF IR JSPS JWST LAE LOFAR Lyman Alpha Blobs Lyman Alpha Forest M-sigma relation M33 MHD MRI MWA 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

There are no items for the academic year Apr 2026 ~ Mar 2027 .

About the Uchu Forum

The Tsukuba Uchu-Forum are a series of talks, which universities and research institutes in the Tsukuba area participate in. It is an event unique to the Kenkyugakuen-toshi.

Usual place and time:

Every third Tuesday of the month
13:30 ~ 15:00
Center for Computational Sciences, University of Tsukuba, Workshop Room or Seminar room.

View

Full View

Stacked

Compact

Full List

Tags

21cm line AGN AGN feedback AGN jets ALMA Andromeda Astrochemistry B-mode polarization CGM CIB CMB CMZ DLA DM Halo Faraday rotation First star G2 GMC GPU GRB Gaia Galactic Archeology Galactic center Godunov scheme HPC HST Hydra A IGM IMF IR JSPS JWST LAE LOFAR Lyman Alpha Blobs Lyman Alpha Forest M-sigma relation M33 MHD MRI MWA 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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Theoretical AstrophysicsGroup

University of Tsukuba, Center for Computational Sciences

Tsukuba Uchu Forum

The Cosmic Himalayas; An Extreme Quasar Concentration at Cosmic Noon Bridging AGNs,...

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