Using passive tracer particles in simulations, the authors show that star-forming cores in clustered regions have lower filling factors, larger masses and sizes, and more protostars than isolated cores.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Tracking Star-Forming Cores as Mass Reservoirs in Clustered and Isolated Regions Using Numerical Passive Tracer Particles
Using passive tracer particles in simulations, the authors show that star-forming cores in clustered regions have lower filling factors, larger masses and sizes, and more protostars than isolated cores.