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New Study Lowers Star Formation Threshold in Dark Matter Halos to 10 Million Solar Masses

Ethan Nadler's research, now published in The Astrophysical Journal Letters, highlights molecular hydrogen cooling as a key factor and sets the stage for upcoming observational tests by Rubin Observatory and JWST.

Overview

  • Ethan Nadler's study reveals that star formation can occur in dark matter halos as small as 10 million solar masses, significantly lower than the previous threshold of 100 million to 1 billion solar masses.
  • The research emphasizes the role of molecular hydrogen cooling, which enables star formation in lower-mass halos compared to earlier models based on atomic hydrogen cooling.
  • The findings, published in *The Astrophysical Journal Letters*, were derived using galaxy formation theory and cosmological simulations.
  • Upcoming observations from the Rubin Observatory and the James Webb Space Telescope (JWST) are expected to test these predictions and potentially uncover completely star-free dark matter halos.
  • The discovery of star-free halos, if confirmed, could provide new insights into the nature of dark matter and reshape our understanding of cosmology.

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