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Table 2

Observed parameters of the H13CO+, HN13C and SiO lines.

NGC 1333 L1448-IRS3 VLA 1623 IRAS 20353
Line νlsr Δν νlsr Δν νlsr Δν νlsr Δν
(km s-1) (km s-1) (K) (km s-1) (km s-1) (K) (km s-1) (km s-1) (K) (km s-1) (km s-1) (K)

H13CO+ (1  →  0) 6.94(2) 0.94(4) 0.696(9) 4.1090(5) 0.805(9) 0.91(2) 2.57(2) 0.60(5) 0.60(5) 2.637(4) 0.56(1) 0.97(1)
7.80(1) 0.71(2) 1.022(9) 4.641(2) 0.736(6) 2.00(2) 3.467(5) 0.74(1) 2.61(5) 3.00(3) 0.54(9) 0.11(1)
5.231(4) 0.746(9) 0.72(2)
H13CO+ (4  →  3) 6.91(2) 0.84(7) 0.29(1) 3.97(4) 1.00(8) 0.14(2) 2.6(1) 0.9(4) 0.17(5) 2.62(5) 0.4(1) 0.051(4)
7.81(9) 0.6(2) 0.06(1) 4.73(2) 0.75(3) 0.39(2) 3.35(2) 1.1(2) 0.47(5)  ~3.1 ...  ≤0.027
5.437(7) 0.72(6) 0.20(2)
HN13C (1  →  0) 6.87(3) 0.84(7) 0.24(1) 4.0(1) 0.5(1) 0.16(1)  ~2.6 ...  ≤0.044 2.66(2) 0.49(3) 0.46(1)
7.90(2) 0.87(4) 0.38(1) 4.7(1) 0.9(1) 0.97(1) 3.58(2) 0.71(6) 0.42(4) 3.1(1) 0.7(2) 0.13(2)
5.5(1) 0.7(1) 0.20(1)
HN13C (4  →  3)  ~6.9 ...  ≤0.032  ~4.0 ...  ≤0.032  ~2.6 ...  ≤0.13  ~2.6 ...  ≤0.040
 ~7.8 ...  ≤0.032  ~4.7 ...  ≤0.032  ~3.5 ....  ≤0.13  ~3.1 ...  ≤0.040
 ~5.4 ...  ≤0.032
SiO (2  →  1) 7.1(2) 3.4(4) 0.10(2)  ~4.0 ...  ≤0.019 2.9(1) 1.3(3) 0.08(2)  ~2.6 ...  ≤0.034
7.83(1) 0.63(4) 0.31(2) 4.545(4) 0.499(9) 0.36(1) ... ... ...  ~3.1 ...  ≤0.034
 ~5.4 ...  ≤0.019
SiO (8  →  7)  ~6.9 ...  ≤0.031  ~4.0 ...  ≤0.033  ~2.6 ...  ≤0.049
 ~7.8 ...  ≤0.031  ~4.7 ...  ≤0.033  ~3.1 ...  ≤0.049
 ~5.4 ...  ≤0.033

Notes. For the peak intensity, , the number in brackets shows the estimated error on the last digit, estimated by the 1σ noise level. For the position, νlsr, and linewidth, Δν, the errors on the last digit quoted are the values given by the fitting routine “minimize” in the CLASS analysis software, which may underestimate the true errors as they do not take into account, for example, uncertainties in the inputs to the fitting routine. The upper limits of the line intensities correspond to the 3σ noise level in the spectra when smoothed to a velocity resolution of  ~0.2 km s-1. At this velocity resolution there should be 3–4 channels contained within the line, which should be sufficient to estimate the peak intensity.

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