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Table 5

Line fluxes and ratios for one position in the globule head.

Instrument Species I(Θ = 20″) I(Θ = 20″) Ratio
[K km s−1] [erg s−1 cm−2 sr−1]
HIFI [C II] 158 μm 153.5 1.08E-03
PACS [O I] 145 μm 25.5 2.29E-04
upGREAT [O I] 63 μm 6.3 6.85E-04
SPIRE [C I] 2–1 7.4 4.04E-06
SPIRE [C I] 1–0 10.2 1.25E-06
upGREAT 12CO 16→15 1.1 7.03E-06
SPIRE 12CO 13→12 9.3 3.19E-05
SPIRE 12CO 12→11 14.9 4.02E-05
SPIRE 12CO 11→10 20.5 4.27E-05
SPIRE 12CO 10→9 26.4 4.13E-05
SPIRE 12CO 9→8 31.7 3.62E-05
SPIRE 12CO 8→7 45.1 3.62E-05
SPIRE 12CO 7→6 51.3 2.76E-05
SPIRE 12CO 6→5 68.2 2.31E-05
SPIRE 12CO 5→4 91.8 1.80E-05
SPIRE 12CO 4→3 104.6 1.05E-05
SPIRE 13CO 9→8 2.6 2.61E-06
SPIRE 13CO 8→7 5.5 3.86E-06
SPIRE 13CO 7→6 9.0 4.24E-06
SPIRE 13CO 6→5 11.1 3.30E-06
SPIRE 13CO 5→4 19.9 3.41E-06
SPIRE [C I] 2–1/1–0 3.23
SPIRE 12CO 8–7/7–6 1.19
SPIRE 12CO 6–5/5–4 1.71
SPIRE 12CO 5–4/4–3 1.94
SPIRE 13CO 8–7/7–6 0.91
SPIRE 13CO 6–5/5–4 0.97

Notes. The fluxes are given in erg s−1 cm−2 sr−1, the ratios are determined from these fluxes for the SPIRE central pixel in the globule head (RA(2000) = 20h33m50s, Dec(2000) = 40°08′36″). All data points have the same angular resolution of 20″. The absolute error for the SPIRE data for the [C I] lines and CO J ≤ 8 is 2.5–3.1E07 erg s−1 cm−2 sr−1 and for J > 8 ~9E07 erg s−1 cm−2. The low- and mid-J CO data have a resolution of ~30–40″ so that we only use line ratios.

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