The D/H ratio in Titan’s acetylene from high spectral resolution IRTF/TEXES observations

Author:

Bézard B.ORCID,Nixon C.A.,Vinatier S.,Lellouch E.,Greathouse T.,Giles R.,Lombardo N.A.,Jolly A.

Funder

CNES

INSU

Publisher

Elsevier BV

Reference56 articles.

1. D/H ratio of Titan from observations of the Cassini/composite infrared spectrometer;Abbas;Astrophys. J.,2010

2. Titan’s aerosol and stratospheric ice opacities between 18 and 500 μm: Vertical and spectral characteristics from Cassini CIRS;Anderson;Icarus,2011

3. The D/H ratio in Titan’s acetylene from high spectral resolution IRTF/TEXES observations: TEXES spectra of Titan and 10 Hygiea. Mendeley data, v1;Bézard,2024

4. Detection of 13CH3D on Titan;Bézard;Icarus,2007

5. On the H2 abundance and ortho-to-para ratio in Titan’s troposphere;Bézard;Icarus,2020

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