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Molecular hydrogen jets and outflows in the Serpens South filamentary cloud
Astronomy and Astrophysics
We aimed to map the jets and outflows from the Serpens South star forming region and find an empirical relationship between the magnetic field and outflow orientation. Near-infrared H2 v=1-0 S(1) 2.122μm -line imaging of the ∼ 30'-long filamentary shaped Serpens South star forming region was carried out. K s broadband imaging of the same region was used for continuum subraction. Candidate driving sources of the mapped jets/outflows are identified from the list of known protostars and youngdoi:10.1051/0004-6361/201218845 fatcat:at44zeu2nnfpvd5iia3gusejq4