Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Carbon monoxide isotope fractionation in the dust cloud Lynds 134

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157476· OSTI ID:5543205
Prior observations of isotopically substituted CO in Lynds 134 are used to discuss the spatial behavior of the (CO)/(/sup 13/CO) abundance ratio as a function of visual extinction in the cloud. (CO)/(/sup 13/CO) is determined from both LTE and non-LTE evaluations of the double ratio (/sup 13/CO)/: C/sup 18/O) by subsequent application of an assumed constant, terrestrial oxygen isotope ratio. It is found that (CO)/(/sup 13/CO) is roughly terrestrial toward the central regions of L134 where A/sub ..nu../> or approx. =7 mag, and decreases in the cloud periphery where A/sub ..nu../ is lower. These results are in qualitative agreement with theoretical expectation for a low-temperature, chemically fractionated dark cloud, in which preferential /sup 13/CO enhancement is driven in low-extinction regions by the charge exchange /sup 13/C/sup +/+/sup 12/CO..-->../sup 12/C+/sup 13/CO. The impact of this result on previous studies of the carbon isotope ratio (/sup 12/C)/(/sup 13/C) in the sense interstellar medium is discussed.
Research Organization:
Rensselaer Polutechnic Institute/The Aerospace Corporation
OSTI ID:
5543205
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 233:4; ISSN ASJOA
Country of Publication:
United States
Language:
English