Dynamics of atmospheres with a non-dilute condensible component
Proceedings of the Royal Society of London. Series A, Mathematical and physical sciences Royal Society, The 472 (2016) 20160107
ALMA OBSERVATIONS OF HCN AND ITS ISOTOPOLOGUES ON TITAN
Astronomical Journal American Astronomial Society 152:42 (2016) 1-7
Abstract:
All rights reserved.We present sub-millimeter spectra of HCN isotopologues on Titan, derived from publicly available ALMA flux calibration observations of Titan taken in early 2014. We report the detection of a new HCN isotopologue on Titan, H13C15N, and confirm an earlier report of detection of DCN. We model high signal-to-noise observations of HCN, H13CN, HC15N, DCN, and H13C15N to derive abundances and infer the following isotopic ratios: 12C/13C = 89.8 ±2.8, 14N/15N = 72.3 ±2.2, D/H = (2.5 ± 0.2) ×10-4, and HCN/H13C15N = 5800 ±270 (1σ errors). The carbon and nitrogen ratios are consistent with and improve on the precision of previous results, confirming a factor of ∼2.3 elevation in 14N/15N in HCN compared to N2 and a lack of fractionation in 12C/13C from the protosolar value. This is the first published measurement of D/H in a nitrile species on Titan, and we find evidence for a factor of ∼2 deuterium enrichment in hydrogen cyanide compared to methane. The isotopic ratios we derive may be used as constraints for future models to better understand the fractionation processes occurring in Titan's atmosphere.Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 458:3 (2016) 2405-2422
New use of global warming potentials to compare cumulative and short-lived climate pollutants
Nature Climate Change Nature Publishing Group 6:8 (2016) 773-776