First detection of 13C17O in a protoplanetary disk indicates the HD 163296 disk's CO gas mass is 3.5 times larger than previously benchmarked models, supporting 13C17O as an optically thin mass tracer.
T., Fedele, D., Hogerheijde, M
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The First Detection of 13C17O in a Protoplanetary Disk: a Robust Tracer of Disk Gas Mass
First detection of 13C17O in a protoplanetary disk indicates the HD 163296 disk's CO gas mass is 3.5 times larger than previously benchmarked models, supporting 13C17O as an optically thin mass tracer.