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Signatures of warm carbon monoxide in protoplanetary discs observed with Herschel SPIRE

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Figure

Table 1. Key parameters of the sources. The Herbig Ae/Be discs with and without flaring, respectively, are listed first, followed by theT Tauri discs
Table 2. SPIRE FTS observational details. The 12 targets in the first segment of the table were observed as part of Herschel programmeGT1 golofs01 4, HD 179218 and HD 50138 were observed under programme GT2 jbouwman 3, and the 4 targets in the last segment
Figure 1. Background-subtracted SPIRE spectra of all sources studied in this paper. The high frequency end of SLW data (>960 GHz)is not shown, because they are noisier than data from the overlapping part of SSW
Figure 2. SPIRE spectra of sources with more than three spectral lines detected at ⩾3σ
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