Why Are (Almost) All the Protostellar Outflows Aligned in Serpens Main?
We present deep 1.4–4.8 μ m JWST-NIRCam imaging of the Serpens Main star-forming region and identify 20 candidate protostellar outflows, most with bipolar structure and identified driving sources. The outflow position angles (PAs) are strongly correlated, and they are aligned within ±24° of the majo...
| Autors principals: | , , , , , , |
|---|---|
| Format: | Article |
| Idioma: | English |
| Publicat: |
IOP Publishing
2024-01-01
|
| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ad5a02 |