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Emission structure of the ¹²CO molecule is more complex. None of the ¹²CO lines is a simple Gaussian, and a broader emission is visible in the wings on both sides. Moreover, line profiles vary considerably in shape at differ­ent points of the ASO1 map. Fig. 4 shows two spectra ob­served in the Southern and Northern parts. The deviation of the profiles can be quantified by looking at the value of J Tdv on the blue - and red sides of the lines (where the "blue" and "red" are relative to the central velocity of -51,5 km/s). The observed deviations may be due to superposi­tion of separate velocity components. We can recognize four velocity ranges on the profiles where the valuej Tdv varies around the whole ASO1 object. Fig. 5 shows maps of the ¹²CO molecule radiation in different velocity ranges. We try to identify different velocity components of the molecular emission as those associated with outflows. The bipolar out­flows can be seen at the velocity — position plot (Fig. 6) for ¹²CO and ¹³CO along the outflow axis with the center at RA(1950) = 00^h42^m05^s, Dec. (1950) = 55°3l'00" (see the vertical section in Fig. 1).We can separate two bipolar out­flows originating from the common point that is coincident with the peak of the integrated emission in the line of ¹³CO.

We have named the two components of the bipolar out­flow the "high-velocity" and "low-velocity" lobes. The "low-velocity" lobe can be identified below 1.5 km/s with re­spect to central velocity. It is marked with "L" in Fig. 6. The "high-velocity" lobe is seen at greater than 1.5 km/s (with respect to central velocity) and has been marked in Fig. 6 as "H"