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We report the detection in the envelope of the C-rich star IRC +10216 of four series of lines with harmonically related frequencies: B1389, B1390, B1394, and B1401. The four series must arise from linear molecules with mass and size close to those of C 6 H and C 5 N. Three of the series have half-integer rotational quantum numbers; we assign them to the 2 Δ and 2 Σ − vibronic states of C 6 H in its lowest (ν 11 ) bending mode. The fourth series, B1389, has integer J with no evidence of fine or hyperfine structure; it has a rotational constant of 1388.860(2) MHz and a centrifugal distortion constant of 33(1) Hz; it is almost certainly the C 5 N − anion.
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