The ALMA Early Science View of FUor/EXor objects. III. The Slow and Wide Outflow of V883 Ori
arXiv:1703.07006 · doi:10.1093/mnras/stx703
Abstract
We present Atacama Large Millimeter/ sub-millimeter Array (ALMA) observations of V883 Ori, an FU Ori object. We describe the molecular outflow and envelope of the system based on the CO and CO emissions, which together trace a bipolar molecular outflow. The CO emission traces the rotational motion of the circumstellar disk. From the CO blue-shifted emission, we estimate a wide opening angle of 150 for the outflow cavities. Also, we find that the outflow is very slow (characteristic velocity of only 0.65 km~s), which is unique for an FU Ori object. We calculate the kinematic properties of the outflow in the standard manner using the CO and CO emissions. In addition, we present a P Cygni profile observed in the high-resolution optical spectrum, evidence of a wind driven by the accretion and being the cause for the particular morphology of the outflows. We discuss the implications of our findings and the rise of these slow outflows during and/or after the formation of a rotationally supported disk.
12 pages, 7 figures, 2 tables. Accepted
References in corpus (9)
- The distance to the Orion Nebula
- The Evolution of Outflow-Envelope Interactions in Low-Mass Protostars
- Imaging the water-snow line during a protostellar outburst
- The Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models
- Modeling jet and outflow feedback during star cluster formation
- The ALMA Early Science view of FUor/EXor objects. I. Through the looking-glass of V2775 Ori
- The ALMA Early Science View of FUor/EXor objects. II. The Very Wide Outflow Driven by HBC 494
- High Resolution Optical and NIR Spectra of HBC 722
- The Winds from HL Tau
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