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Table 2

Parameters of C2H line fitting results.

KNOT α 2000 δ 2000 ηf ×(TexTbg) × τstr (vvsys)str FHWM str τ str
h m s o (K) (km s-1) (km s-1)

SB-I 02h:42m:40.65s −00°01′01.2″ (2.8 ± 1.0) × 10-1 19 ± 8 139 ± 22 0.2 ± 0.6
SB-II 02h:42m:40.31s −00°01′01.9″ (5.3 ± 0.7) × 10-1 79 ± 3 63 ± 11 0.1 ± 0.2
SB-III 02h:42m:40.85s −00°00′33.1″ (6.6 ± 0.5) × 10-1 −20 ± 2 34 ± 10 0.1 ± 0.3
OUT-I 02h:42m:40.76s −00°00′48.0″ (6.8 ± 0.3) × 10-1 −41 ± 3 126 ± 10 0.1 ± 0.1
OUT-II 02h:42m:40.59s −00°00′49.0″ (4.1 ± 1.1) × 10-1 −13 ± 5 135 ± 16 0.1 ± 1.9
OUT-III 02h:42m:40.96s −00°00′45.5″ (5.4 ± 1.6) × 10-1 −37 ± 5 101 ± 12 1.3 ± 0.7

Notes. All the line parameters correspond to the strongest C2H(1−0) line (J = 3/2−1/2, F = 2−1) and are derived according to the procedure described in Sect. 3.3 as follows: Tex is the excitation temperature, Tbg is the background temperature (2.73 K), ηf is the unknown filling factor of the emission, (vvsys)str is the velocity centroid of the line relative to = 1136 km s-1, FHWMstr is the half width at half maximum of the line, and τstr is the estimated peak opacity.

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