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.
C., Le, D., & Jimenez Vela, L
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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.