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Carbon Monoxide in low-mass dwarf stars
Hugh R. A. Jones, Yakiv Pavlenko, Serena Viti +4
We compare high resolution infrared observations of the CO 3-1 bands in the 2.297-2.310 micron region of M dwarfs and one L dwarf with theoretical expectations. We find a good matc…
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…
Calculated spectra for HeH+ and its effect on the opacity of cool metal poor stars
Elodie A. Engel, Natasha Doss, Gregory J. Harris +1
The wavelength and Einstein A coefficient are calculated for all rotation-vibration transitions of HeH, HeH, HeH and HeH, giving a c…
Deuterated hydrogen chemistry: Partition functions, Equilibrium constants and Transition intensities for the H3+ system
Jayesh Ramanlal, Jonathan Tennyson
H3+ and the deuterated isotopomers are thought to play an important role in interstellar chemistry. The partition functions of H3+, D2H+ and D3+ are calculated to a temperature of…