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Filament Accretion and Fragmentation in the Perseus Molecular Cloud

Observations suggest that filaments in molecular clouds can grow by mass accretion while forming cores via fragmentation. Here, we present one of the first large-sample studies of filament accretion using velocity gradient measurements of star-forming filaments on the ∼0.05 pc scale with NH _3 obser...

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Detaylı Bibliyografya
Asıl Yazarlar: Michael Chun-Yuan Chen, James Di Francesco, Rachel K. Friesen, Jaime E. Pineda, Paola Caselli, Adam Ginsburg, Helen Kirk, Anna Punanova, The GAS Collaboration
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2024-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Online Erişim:https://doi.org/10.3847/1538-4357/ad88e8
Etiketler: Etiketle
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