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Star Formation in Galaxies Tied to Gas Location, Not Quantity

New findings from the WALLABY survey using ASKAP telescope reveal that the spatial distribution of atomic hydrogen gas within galaxies drives star formation.

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Overview

  • The WALLABY survey, conducted with CSIRO’s ASKAP telescope, mapped atomic hydrogen gas in nearly 1,000 galaxies with unprecedented detail.
  • Researchers found that star formation correlates with the location of atomic hydrogen gas, particularly within star-forming regions, rather than the total gas quantity in a galaxy.
  • Gas located in the outer regions of galaxies contributes minimally to star formation, emphasizing the importance of spatial concentration within galactic disks.
  • The study challenges traditional models of star formation that linked higher gas mass directly to increased star creation rates.
  • Published in the journal PASA on May 21, 2025, this research provides new insights into galaxy evolution and refines theoretical frameworks for cosmic development.