Comparison of the gas molecular content in the hot-core and outflow components at N1SE1 and N1NW3 amongst each other and with positions N1S and N1S1, which were analysed in Paper I. Rows a–b: abundances with respect to H₂ normalised to the value derived at N1S, where H₂ column densities were derived from a) dust emission at 242 GHz and b) C¹⁸O for all components but N1S, for which the value from dust emission was used in both rows. Component N1NW3:OF is not shown, because C¹⁸O is difficult to identify due to contamination by another molecule. Rows c–d: same as (b), but abundances with respect to C₂H₅CN and CH₃OH are shown, respectively. In all panels, hatched bars indicate when the rotational temperature in a population diagram (PD) was fixed (NH₂CN at N1SE1:HC and CH₃SH at N1S), the molecule was detected but a PD could not be derived (NH₂CHO at N1SE1:OF), or only an upper limit for the rotational temperature in the PD was derived. Empty bars show upper limits. HC₅N and OCS are not shown as we do not have the column densities of the two molecules at N1S.