Implication of Formation Mechanisms of HC5N in TMC-1 as Studied by 13C
  Isotopic Fractionation
  We observed the J = 9-8 and 16-15 rotational transitions of the normal
species and five 13C isotopologues of HC5N to study its formation mechanisms
toward the cyanopolyyne peak in Taurus Molecular Cloud-1, with the 45-m radio
telescope of Nobeyama Radio Observatory. We detected the five 13C isotopologues
with high signal-to-noise ratios between 12 and 20, as well as the normal
species. The abundance ratios of the five 13C isotopologues of HC5N are found
to be 1.00:0.97:1.03:1.05:1.16 (0.19) for
[H13CCCCCN]:[HC13CCCCN]:[HCC13CCCN]:[HCCC13CCN]:[HCCCC13CN]. We do not find any
significant differences among the five 13C isotopologues. The averaged
[HC5N]/[13C isotopologues] abundance ratio is determined to be 94 (6), which is
slightly higher than the local interstellar elemental 12C/13C ratio of 60-70.
Possible formation pathways are discussed on the basis of these results.
