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December 3, 2025Monthly Notices of the Royal Astronomical SocietyOpen Access

The Pandora project. II: how non-thermal physics drives bursty star formation and temperate mass-loaded outflows in dwarf galaxies

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Authors

SMSergio Martin-AlvarezDSDebora SijackiMHMartin G. Haehnelt

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Overview

Analysis reveals magnetic fields and baryons drive bursty star formation and mass-loaded outflows in dwarf galaxies, highlighting their role in galaxy evolution.

Key Points

  • Star formation and outflow dynamics are driven by non-thermal processes including magnetic fields.
  • Magnetic fields and baryons play essential roles in regulating star formation and outflows in dwarf galaxies.
  • Simulations of dwarf galaxies demonstrate the impact of non-thermal physics on metal retention and outflow characteristics.
  • These findings underline the need to include non-thermal physics in galaxy formation models for accurate predictions.

Cite This Study

Martin-Alvarez et al. (2025) studied this question.

synapsesocial.com/papers/694025742d562116f28fde8chttps://doi.org/10.1093/mnras/staf2106
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