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Table 1

Properties of the selected observed lines.

Species Transition Frequency(a) (MHz) Beff Tmb,peak (K) rms (mK) VLSR(b) (km s−1) Δυ(b) (km s–1) Tmb (K km s–1)
L1544
CCH N=1–0, J=1/2–1/2, F=1–0 87446.47(1) 0.52 0.96(3) 27 7.24 0.39 0.40(2)
13CCH N=1–0, J=3/2–1/2, F1=2–1, F=5/2–3/2 84119.33(2) 0.53 0.039(5) 7 7.31 0.32 0.013(2)
C13CH N=1–0, J=3/2–1/2, F1=2–1, F=5/2–3/2 85229.335(4) 0.53 0.089(6) 9 7.35 0.32 0.030(3)
CCD N=1–0, J=1–0, F1 =3/2–1/2, F=3/2–3/2 72101.811(5) 0.54 0.19(1) 24 7.23 0.39 0.078(9)
H13CN J=1–0, F=0–1 86342.2543(3) 0.53 0.22(1) 18 7.21 0.39 0.091(7)
DCN J=1–0, F=0–1 72417.03(1) 0.54 0.69(2) 23 7.14 0.37 0.27(1)
H13CO+ J=1–0 86754.288(5) 0.53 1.38(4) 20 7.13 0.52 0.77(4)
HC18O+ J=1–0 85162.223(5) 0.53 0.229(6) 9 7.18 0.38 0.093(4)
DCO+ J=1–0 72039.3124(8) 0.54 2.44(5) 25 7.12 0.60 1.55(4)
HN13C J=1–0, F1=0–1, F2=1–2, F=1–2 87090.675(3) 0.52 0.27(3) 25 7.92 0.24 0.07(2)
DNC J,I,F=1,2,1–0,2,2; 1,2,1–0,0,0 76305.513(1) 0.54 0.99(2) 26 7.90 0.40 0.42(2)
HH211
CCH N=1–0, J=3/2–1/2, F=1–1 87284.11(1) 0.52 0.50(1) 27 9.02 0.54 0.29(1)
13CCH N=1–0, J=3/2–1/2, F1=1–0, F=3/2–1/2 84153.31(2) 0.53 0.016(4) 6 9.07 0.4 0.007(2)
C13CH N=1–0, J=3/2–1/2, F1=2–1, F=5/2–3/2 85229.335(4) 0.53 0.032(4) 8 9.10 0.53 0.018(4)
CCD N=1–0, J=1–0, F1 =3/2–1/2, F=5/2–3/2 72107.721(3) 0.54 0.37(5) 28 9.10 0.45 0.18(3)
H13CN J=1–0, F=2–1 86340.1666(1) 0.53 0.45(2) 23 9.05 0.61 0.29(2)
DCN J=1–0, F=0–1 72417.03(1) 0.54 0.35(2) 22 9.06 0.50 0.18(4)
H13CO+ J=1–0 86754.288(5) 0.53 1.95(1) 24 8.97 0.60 1.24(2)
HC18O+ J=1–0 85162.223(5) 0.53 0.153(4) 8 9.03 0.53 0.087(5)
DCO+ J=1–0 72039.3124(8) 0.54 3.01(1) 22 9.04 0.74 2.38(2)
HN13C J=1–0 87090.825(4) 0.52 0.58(1) 27 9.09 0.71 0.46(1)
HN13C J=1–0, F1=0–1 F2=1–2, F =1–2 87090.675(3) 0.52 0.090(5) 27 9.78 0.35 0.034(7)
DNC J,I,F=1,2,1–0,2,2; 1,2,1–0,0,0 76305.513(1) 0.54 0.56(3) 31 9.90 0.38 0.22(4)

Notes. Numbers in brackets give the uncertainty on the last digit. (a)Extracted from Cologne Database for Molecular Spectroscopy (Müller et al. 2001). (b)The uncertainties of the fits are smaller than the velocity resolution. Therefore, the error on VLSR and Δυ are given by the observed spectral resolution, 0.07 km s−1.

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