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Fig. 2.

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Spectra of CH and H2O lines toward PKS 1830−211 NE and SW images (left, middle, respectively), and toward B 0218+357(SW) (right) observed by ALMA at different epochs. The spectra are colored by dates, as is indicated in the top left and top right boxes. The hyperfine structure of each CH Λ-doublet is indicated at the bottom of spectra. The spectrum of the H218O isotopolog, taken on 2014 May 05, is also shown for PKS 1830−211(SW) (top-middle box, in light blue). A zoom on the weak v ∼ +170 km s−1 velocity component is shown for PKS 1830−211(SW), with the 2016 averaged spectra (in purple) instead of that taken on 2016 March 05.

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