Abundance and excitation of molecular anions in interstellar clouds

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Fig. 3

Lines of C₈N⁻ observed toward TMC-1 CP and lines of the nitrile anions C₃N⁻ and C₅N⁻ observed toward TMC-1 CP and Lupus-1A using the Yebes 40 m and IRAM 30 m telescopes. See the line parameters in Table A.1.

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