Abstract
The high-mass star-forming region IRAS 17333-3606 has been mapped in the 13CO (J = 2–1) and C18O (J = 2–1) lines in the submillimeter wavelength range using the APEX (Chile) radio telescope. The analysis of the low-velocity part of the molecular outflow has been carried out, and the main parameters of the outflow have been determined. We have used a novel approach for calculating parameters of the low-velocity part of bipolar molecular outflows in molecular clouds. The approach excludes the influence of the surrounding cloud on the parameters of the outflow. The mass of the low-velocity part is much greater than that of the high-velocity part of the molecular outflow, while their energies are comparable. The core of the young stellar object is significantly deformed by the impact of the bipolar outflow.
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Original Russian Text © O.V. Antyufeyev, V.M. Shulga, I.I. Zinchenko, 2016, published in Kinematika i Fizika Nebesnykh Tel, 2016, Vol. 32, No. 6, pp. 20–29.
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Antyufeyev, O.V., Shulga, V.M. & Zinchenko, I.I. Bipolar molecular outflow in IRAS 17233-3606. Kinemat. Phys. Celest. Bodies 32, 276–282 (2016). https://doi.org/10.3103/S0884591316060027
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DOI: https://doi.org/10.3103/S0884591316060027