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...
Saved in:
| Main Authors: | Michael Chun-Yuan Chen, James Di Francesco, Rachel K. Friesen, Jaime E. Pineda, Paola Caselli, Adam Ginsburg, Helen Kirk, Anna Punanova, The GAS Collaboration |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad88e8 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Magnetic Field in Quiescent Star-forming Filament G16.96+0.27
by: Qi-Lao Gu, et al.
Published: (2024-01-01) -
The JCMT BISTRO Survey: The Magnetic Fields of the IC 348 Star-forming Region
by: Youngwoo Choi, et al.
Published: (2024-01-01) -
A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey
by: Jintai Wu, et al.
Published: (2024-01-01) -
Extinction of Taurus, Orion, Perseus and California Molecular Clouds Based on the LAMOST, 2MASS, and Gaia Surveys. II. The Extinction Law
by: ZheTai Cao, et al.
Published: (2024-01-01) -
The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud
by: Dongting Yang, et al.
Published: (2024-01-01)