Multi-epoch subarcsecond [Fe II] spectroimaging of the DG tau outflows with NIFS - II. On the nature of the bipolar outflow asymmetry
The origin of bipolar outflow asymmetry in young stellar objects (YSOs) remains poorly understood. It may be due to an intrinsically asymmetric outflow launch mechanism, or it may be caused by the effects of the ambient medium surrounding the YSO. Answering this question is an important step in understanding outflow launching. We have investigated the bipolar outflows driven by the T Tauri star DG Tauri on scales of hundreds of astronomical units, using the Near-infrared Integral Field...[Show more]
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_White_Multi-epoch_subarcsecond_[Fe_2014.pdf||2.33 MB||Adobe PDF|
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