1. Molecular Reconnaissance of the β Pictoris Gas Disk with the SMA: A Low HCN/(CO+CO2) Outgassing Ratio and Predictions for Future Surveys
- Author
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Matrà, L, Wilner, DJ, Öberg, KI, Andrews, SM, Loomis, RA, Wyatt, MC, Dent, WRF, Matrà, L [0000-0003-4705-3188], Wilner, DJ [0000-0003-1526-7587], Öberg, KI [0000-0001-8798-1347], Andrews, SM [0000-0003-2253-2270], Loomis, RA [0000-0002-8932-1219], Wyatt, MC [0000-0001-9064-5598], and Apollo - University of Cambridge Repository
- Subjects
molecular processes ,comets: general ,stars: individual (beta Pictoris) ,submillimeter: planetary systems ,circumstellar matter ,planetary systems - 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 $\beta$ Pictoris belt with the Submillimeter Array (SMA), reporting upper limits for CN, HCN, HCO$^+$, N$_2$H$^+$ and H$_2$CO, as well as for H$_2$S, CH$_3$OH, SiO and DCN from archival ALMA data. Non-detections can be attributed to rapid molecular photodissociation due to the A-star's strong UV flux. CN is the longest-lasting and most easily detectable molecule after CO in this environment. We update our NLTE excitation model to include UV fluorescence, finding it plays a key role in CO and CN excitation, and use it to turn the SMA CN/CO flux ratio constraint into an upper limit of $
- Published
- 2018
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