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May 16, 2026The Astrophysical JournalOpen Access

Fragmentation in the Serpens/Aquila Star-forming Region

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Authors

SFSamuel D. FielderHKHelen KirkMDMichael M. Dunham

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Overview

Population study reveals fragmentation patterns in dense cores, suggesting turbulence influences star formation.

Key Points

  • This study aims to analyze the characteristics and fragmentation of dense cores in the Serpens/Aquila star-forming region.
  • Conducted observations with Atacama Large Millimeter/submillimeter Array (ALMA) at 106 GHz
  • Analyzed 100 gravitationally unstable dense cores and their fragmentation into starless and protostellar structures
  • Implemented synthetic observations from turbulent magnetohydrodynamical simulations to predict starless core detections.
  • Identified 66 continuum sources with 2 completely starless and 9 within protostellar cores
  • Predictions from simulations align with the observed detection of 1.19 starless cores
  • Observed an increase in multiplicity at smaller scales corresponding to higher fragmentation in larger structures.

Cite This Study

Fielder et al. (2026) studied this question.

synapsesocial.com/papers/6a0808afa487c87a6a40ae73https://doi.org/10.3847/1538-4357/ae6064
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Also Consider

Synapse has enriched 4 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Observing turbulent fragmentation in simulations: predictions for CARMA and ALMA2011 · 31 citations
  2. 2The Two Micron All Sky Survey (2MASS)2006 · 12,281 citations
  3. 3ALMA Observations of Starless Core Substructure in Ophiuchus2017 · 49 citations
  4. 4The formation of active protoclusters in the Aquila rift: a millimeter continuum view2011 · 156 citations