Rotation in the NGC 1333 IRAS 4C Outflow
نویسندگان
چکیده
منابع مشابه
An S - shaped outflow from IRAS 03256 + 3055 in NGC 1333
The IRAS source 03256+3055 in the NGC 1333 star forming region is associated with extended sub-millimeter emission of complex morphology, showing multiple clumps. One of these is found to coincide with the driving source of a bipolar jet of S-shaped morphology seen in the emission lines of Hα and [SII] as well as in the H2 emission lines in the K-band. Detailed images of the driving source at t...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2018
ISSN: 1538-4357
DOI: 10.3847/1538-4357/aad7ba