Molecular Reconnaissance of the β Pictoris Gas Disk with the SMA: A Low HCN/(CO+CO2 ) Outgassing Ratio and Predictions for Future Surveys
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Abstract
The exocometary origin of CO gas has been confirmed in several extrasolar
Kuiper belts, with CO ice abundances consistent with Solar System comets. We
here present a molecular survey of the
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1538-4357