Herschel/HIFI observations of red supergiants and yellow hypergiants - I. Molecular inventory

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Fig. 9

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Histograms of the peak brightness temperatures as tabulated in Tables 3 and 4, for lines detected in at least 2 sources, normalised by the ¹²CO J = 6−5 intensity of the respective sources. Non-detected lines are not represented in this graph.

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