Bibcode
Yousefi, M.; Bernath, P. F.; Hodges, J.; Masseron, T.
Bibliographical reference
Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 217, p. 416-424.
Advertised on:
9
2018
Citations
36
Refereed citations
34
Description
A new line list for the A2Σ+ -X2
Π electronic transition of OH has been calculated. Line positions
have been taken from the literature and refitted with Western's PGOPHER
program. Line intensities were calculated using a new ab initio
Transition Dipole Moment Function (TDMF) obtained with Molpro 2012. The
new TDMF and the potential functions from LeRoy's RKR program have been
used as input to LeRoy's LEVEL program in order to calculate Transition
Dipole Moment Matrix Elements (TDMMEs). These matrix elements were
transformed from Hund's case (b) to Hund's case (a) as required for the
PGOPHER program using the method of Brooke et al. [JQSRT 2016; 168:
142-157] The line list was calculated with PGOPHER for bands with
v‧ = 0 - 4 in the A2Σ+
state and v″ = 0 - 9 for the X2Π state.
Related projects
Nucleosynthesis and molecular processes in the late stages of Stellar Evolution
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars are important contributors to the enrichment of the
Domingo Aníbal
García Hernández