The interstellar C 18 O / C 17 O ratio in the solar neighbourhood : The ρ Oph cloud ⋆

نویسنده

  • C. Henkel
چکیده

Observations of up to ten carbon monoxide (CO and isotopomers) transitions are presented to study the interstellar CO/CO ratio towards 21 positions in the nearby (d∼140 pc) low-mass star forming cloud ρ Oph. A map of the CO J=1–0 distribution of parts of the cloud is also shown. An average CO/CO isotopomeric ratio of 4.11 ± 0.14, reflecting the O/O isotope ratio, is derived from Large Velocity Gradient (LVG) calculations. From LTE column densities we derive a ratio of 4.17±0.26. These calculations also show that the kinetic temperature decreases from about 30 K in the cloud envelope to about 10 K in the cloud cores. This decrease is accompanied by an increase of the average molecular hydrogen density from 10 cm to >∼10 5 cm. Towards some lines of sight CO optical depths reach values of order unity.

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تاریخ انتشار 2004