Wd. Langer et Aa. Penzias, C-12 C-13 ISOTOPE RATIO IN THE LOCAL INTERSTELLAR-MEDIUM FROM OBSERVATIONS OF (CO)-C-13-O-18 IN MOLECULAR CLOUDS/, The Astrophysical journal, 408(2), 1993, pp. 539-547
The C-12/C-13 isotope ratio is studied in the solar neighborhood from
observations of the (CO)-C-12-O-18 and (CO)-C-13-O-18 J = 1-0 transiti
ons in four interstellar clouds located within 500 pc. Three of these,
B5, B335, and L183 (L134N), are dark clouds not associated with stron
g H II regions, and the fourth is at a position in Orion A relatively
distant from the H II region associated with the KL source. The C-12/C
-13 ratio in these sources (after corrections for a small amount of ra
diative trapping) ranges from 57 to 74, and its weighted average is 62
+/- 4, with thermal noise and line formation uncertainties contributi
ng about equally to the probable error. This ratio is consistent with
the value we previously derived from the (CO)-C-12-O-18/(CO)-C-13-O-18
Galactic gradient, as well as with the most likely range, 60-70, dete
rmined from CH+ absorption measurements in the diffuse cloud zeta Oph.
Thus the most reliable CO and CH+ results are consistent within their
errors. The resulting value indicates moderate chemical evolution in
the local solar neighborhood since the formation of the solar system,
in good agreement with model prediction of the current carbon ratio in
the local interstellar medium.