Turbulence in Zeeman Measurements from Molecular Clouds
Magnetic fields ( B fields) play an important role in molecular cloud fragmentation and star formation but are very difficult to detect. The temporal correlation between the field strength ( B ) and gas density ( n ) of an isolated cloud has been suggested as an indication of the dynamical importanc...
| Egile Nagusiak: | , |
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| Formatua: | Artikulua |
| Hizkuntza: | English |
| Argitaratua: |
IOP Publishing
2023-01-01
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| Saila: | The Astrophysical Journal Letters |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/2041-8213/acc5e8 |