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Table 7

Molecular line emission from the e-EVSa.

Line Instr. S Δυb I
(Jy) (km s−1) (Jy km s−1)
     
CO(1–0) SEST 0.38 6.2
CO(2–1) ALMA 1.38 10.8 16
SEST 1.48 21
CO(3–2) APEX 1.64 35
CO(4–3) APEX 0.86 54
CO(6–5) APEX 0.86 68
13CO(2–1) ALMA 0.54 7.5 4.3
SEST 0.49 8.6
13CO(3–2) APEX 0.37 7.0
C18O(2–1) ALMA 0.06 4.8 0.31
SiO(5–4) ALMA 0.45 9.5 4.5
29SiO(5–4) ALMA 0.17 7.2 1.3
CS(4–3) APEX 0.2 1.9
13CS(5–4) ALMA 0.065 9.6 0.66
SO(55−44) ALMA 0.078 9.2 0.76
SO(56−45) ALMA 0.10 5.8 0.61
OCS(18–17) ALMA 0.016 8.6 0.15
OCS(19–18) ALMA 0.016 7.9 0.13
HCN(3–2) APEX 0.08 1.4
HCO+(3–2) APEX 0.06 1.0
p-H2O(313−220) APEX <3
p-H2CO(303−202) ALMA 0.10 9.3 1.0
p-H2CO(322−221) ALMA 0.034 9.4 0.34
p-H2CO(321−220) ALMA 0.039 7.4 0.31
o-HCO(312−211) ALMA 0.023 8.7 0.21
E-CH3OH(42−31) ALMA 0.051 5.2 0.28
E-CH3OH(8−1−70) ALMA 0.065 6.2 0.43

Notes. (a) The line intensities apply to the velocity interval and region specified in the text for the ALMA data, and within the velocity interval specified in the text for the APEX and SEST data. The single-dish data are observed with the beam positioned at the centre of the source, and the reported intensities are not corrected for the beam response. Flux uncertainties are discussed in Sect. 4.7. (b) FWHM of a Gaussian fit to the line within the given aperture at 1.5 km s−1 resolution.

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