activity
20032025
most citedThe ExoMol database: molecular line lists for exoplanet and other hot atmospheres

545 citations · 847 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025★ 1 cited

VVV-WIT-13: an eruptive young star with cool molecular features

Zhen Guo, Philip Lucas, Sergey N. Yurchenko +27

Here we investigate an infrared eruptive source, identified from the decade-long VISTA Variables in the Via Lactea survey (VVV). We named this target after a group of variable sour…

astro-ph.SR2024

ExoMol Line Lists -- LXII: Ro-Vibrational Energy Levels and Line-Strengths for the Propadienediylidene (C3) in its Ground Electronic State

A. E. Lynas-Gray, O. L. Polyansky, J. Tennyson +2

Improved opacities are needed for modelling the atmospheres and evolution of cool carbon-rich stars and extra-solar planets; in particular, contributions made by the astrophysicall…

astro-ph.SR2020★ 231 cited

The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres

Jonathan Tennyson, Sergei N. Yurchenko, Ahmed F. Al-Refaie +19

The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmospheres. While the data is intended for studies of exoplanets and other astronomic…

astro-ph.GA2016★ 545 cited

The ExoMol database: molecular line lists for exoplanet and other hot atmospheres

Jonathan Tennyson, Sergei N. Yurchenko, Ahmed F. Al-Refaie +16

The ExoMol database (www.exomol.com) provides extensive line lists of molecular transitions which are valid over extended temperatures ranges. The status of the current release of…

astro-ph2004★ 34 cited

The role of HeH+ in cool helium rich white dwarfs

G. J. Harris, A. E. Lynas-Gray, S. Miller +1

HeH is found to be the dominant positive ion over a wide range of temperatures and densities relevant to helium rich white dwarfs. The inclusion of HeH in ionization equili…

astro-ph2003★ 18 cited

The effect of the electron donor H3+ on the pre-main and Main Sequence evolution of low mass zero metallicity stars

G. J. Harris, A. E. Lynas-Gray, S. Miller +1

H3+ has been shown (Lenzuni et al. 1991, ApJS, 76, 759) to be the dominant positive ion, in a zero metallicity gas at low temperature and intermediate to high density. It therefore…