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Diffuse inter-filament gas is likely a key fuel source for massive star formation

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Diffuse inter-filament gas is likely a key fuel source for massive star formation
Foto: Scott Lord / Pexels

Diffuse inter-filament gas is likely a key fuel source for massive star formation. Researchers from Kyushu University have discovered that diffuse gas surrounding dense filaments in a nearby stellar nursery plays a much larger role in star formation than previously recognized.

A apuração publicada por phys.org vira base para uma leitura editorial direta e contextualizada.

Trechos de apoio da pauta: Researchers from Kyushu University have discovered that diffuse gas surrounding dense filaments in a nearby stellar nursery plays a much larger role in star formation than previously recognized. By tracking the movement of gas in the Monoceros R2 hub–filament system, the team found that low-density gas contributes to hub growth both through direct inflow and by replenishing nearby dense filaments.

  • Ponto de atenção: diffuse.
  • Ponto de atenção: inter.
  • Ponto de atenção: filament.

Em resumo, a leitura editorial acompanha o impacto do tema no nicho Ciência.

Artigo originalmente publicado em phys.org
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