ExoMol molecular line lists X: The spectrum of sodium hydride
arXiv:1506.00174 · doi:10.1093/mnras/stv979
Abstract
Accurate and complete rotational, rotational-vibrational and rotational-vibrational-electronic line lists are calculated for sodium hydride: both the NaH and NaD isotopologues are considered. These line lists cover all ro-vibrational states of the ground (~) and first excited (~) electronic states. The calculations use available spectroscopically-determined potential energy curves and new high-quality, \textit{ab initio} dipole moment curves. Partition functions for both isotopologues are calculated and the effect of quasibound states is considered. The resulting line lists are suitable for temperatures up to about 7000~K and are designed for studies of exoplanet atmospheres, brown dwarfs and cool stars. In particular, the NaH band is found to show a broad absorption feature at about 385 nm which should provide a signature for the molecule. All partition functions, lines and transitions are available as Supplementary Information to this article and at \url{www.exomol.com}.
8 pages, 5 figures, 6 tables
References in corpus (4)
- ExoMol molecular line lists V: The ro-vibrational spectra of NaCl and KCl
- ExoMol molecular line lists: IX The spectrum of AlO
- The rovibrational spectrum of BeH, MgH and CaH at high temperatures in the state: a theoretical study
- Exomol molecular line lists VI: A high temperature line list for Phosphorus Nitride
Cited by in corpus (24)
- The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- The ExoMolOP Database: Cross-sections and k-tables for Molecules of Interest in High-Temperature Exoplanet Atmospheres
- Self-luminous and irradiated exoplanetary atmospheres explored with HELIOS
- New Avenues for Thermal Inversions in hot Jupiters
- The ExoMol project: Software for computing large molecular line lists
- ExoMol Line List XXI: Nitric Oxide (NO)
- TRIDENT: A Rapid 3D Radiative Transfer Model for Exoplanet Transmission Spectra
- Laboratory spectra of hot molecules: data needs for hot super-Earth exoplanets
- A blue depression in the optical spectra of M dwarfs
- Low-Temperature Gas Opacities with AESOPUS 2.0
- ExoMol line lists -- XLI. High-temperature molecular line lists for the alkali metal hydroxides KOH and NaOH
- Data availability and requirements relevant for the Ariel space mission and other exoplanet atmosphere applications
- Predicted Landé -factors for open shell diatomic molecules
- Observability of silicates in volatile atmospheres of super-Earths and sub-Neptunes
- The NewEra model grid
- 3D Stagger model atmospheres with FreeEOS I. Exploring the impact of microphysics on the Sun
- ExoMol line lists -- XLVII. Rovibronic molecular line list of the calcium monohydroxide radical (CaOH)
- MARVEL analysis of the measured high-resolution rovibronic spectra of the calcium monohydroxide radical (CaOH)
- Characterising the Atmosphere of 55 Cancri e: 1D Forward Model Grid for Current and Future JWST Observations
- Conditions for radiative zones in the molecular hydrogen envelope of Jupiter and Saturn: The role of alkali metals
- The model for cloudy substellar atmospheres: A grid of self-consistent substellar atmosphere models with microphysical cloud formation
- Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
- A grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres
- A new look into the atmospheric composition of WASP-39 b