| Tartalmi leírás: |
Eruptive young stars can sometimes be accompanied by bipolar molecular outflows which can significantly alter the system’s environment. I studied the outflow properties of Haro 5a IRS, a FUor-like protobinary system, based on ALMA observations. I focused on 12CO, 13CO and C18O detections of molecular outflows emanating from the system. I measured their geometrical properties, and estimated their physical properties which I then put into context.
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