Inclination-angle of the outflow in IRAS 05553+1631: A method to correct the projection effect
Shuo Kong, Yuefang Wu

TL;DR
This paper introduces a new method to accurately determine the inclination angle of outflows in star-forming regions, correcting projection effects to improve the calculation of outflow parameters.
Contribution
A novel approach using contour diagrams and equations to directly calculate the inclination angle of bipolar outflows, enhancing the accuracy of derived physical parameters.
Findings
Inclination angles of 73° and 78° were determined for the outflow in IRAS 05553+1631.
Corrected parameters significantly differ from initial estimates assuming 45°, affecting timescales and energetics.
The method reduces uncertainties in outflow property calculations by accounting for projection effects.
Abstract
A mapping study of IRAS 05553+1631 was performed with 12CO J=3-2 and 13CO J=2-1 lines observed by the KOSMA 3 m-telescope. A core with a size of 0.65 pc and with a LTE mass of 120 M\odot was defined by the mapping with 13CO J=2-1 line. We have identified a bipolar outflow with 12CO J=3-2. For accuracy in the calculation of outflow parameters, overcoming the projection effect is important. We propose a new method to directly calculate the inclination-angle {\theta}. We establish two basic equations with the help of outflow contour diagram and finally obtain the "angle function" and the "angle equation" to derive {\theta}. We apply our method to the outflow of IRAS 05553+1631, finding that {\theta}blue is 73\circ and {\theta}red is 78\circ. Compared to the parameters initially estimated under an assumption of 45\circ inclination-angle, the newly derived parameters are changed with…
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