SPH simulations of filament fragmentation indicate isotopic inhomogeneities from 1 pc filaments survive in cores at reduced levels and potentially reach circumstellar disks.
C., Lugaro, M., & Sch¨ onb¨ achler, M
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Formation of Isotopically Heterogeneous Molecular Cloud Cores in Filamentary Molecular Clouds
SPH simulations of filament fragmentation indicate isotopic inhomogeneities from 1 pc filaments survive in cores at reduced levels and potentially reach circumstellar disks.