https://www.iac.es/es/ciencia-y-tecnologia/publicaciones/headless-tadpole-galaxy-high-gas-phase-metallicity-ultra-diffuse-galaxy-ugc-2162?base_route_name=entity.node.canonical&overridden_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-15&page_manager_page_variant_weight=-7
The cosmological numerical simulations tell us that accretion of external metal-poor gas drives star formation (SF) in galaxy disks. One the best pieces of...
tadpole galaxygas phaseheadlesshighmetallicity
https://www.iac.es/es/ciencia-y-tecnologia/publicaciones/headless-tadpole-galaxy-high-gas-phase-metallicity-ultra-diffuse-galaxy-ugc-2162
The cosmological numerical simulations tell us that accretion of external metal-poor gas drives star formation (SF) in galaxy disks. One the best pieces of...
tadpole galaxygas phaseheadlesshighmetallicity
https://www.iac.es/en/science-and-technology/publications/headless-tadpole-galaxy-high-gas-phase-metallicity-ultra-diffuse-galaxy-ugc-2162?base_route_name=entity.node.canonical&overridden_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-15&page_manager_page_variant_weight=-7
The cosmological numerical simulations tell us that accretion of external metal-poor gas drives star formation (SF) in galaxy disks. One the best pieces of...
tadpole galaxygas phaseheadlesshighmetallicity