Bibcode
Fernando, A. M.; Bernath, P. F.; Hodges, J. N.; Masseron, T.
Referencia bibliográfica
Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 217, p. 29-34.
Fecha de publicación:
9
2018
Número de citas
22
Número de citas referidas
21
Descripción
A new linelist for the
A3Π-X3Σ- electronic transition
of NH has been prepared using line positions from the literature and
calculated line intensities. High level ab initio calculations were
performed with the MOLPRO program to obtain the A-X transition dipole
moment function. Potential energy curves and line strengths were
calculated with Le Roy's RKR1 and LEVEL programs. Line intensities and
Einstein A values were calculated with Western's PGOPHER program after
converting the Hund's case (b) output of LEVEL to Hund's case (a) input
needed for PGOPHER. The Herman-Wallis effect is included in the Einstein
A calculations of the bands for the levels with v‧ = 0
- 2 and v″ = 0 - 6 .
Proyectos relacionados
Nucleosíntesis y procesos moleculares en los últimos estados de la evolución estelar
Las estrellas de masa baja e intermedia (M < 8 masas solares, Ms) representan la mayoría de estrellas en el Cosmos y terminan sus vidas en la Rama Asintótica de las Gigantes (AGB) - justo antes de formar Nebulosas Planetarias (NPs) - cuando experimentan procesos nucleosintéticos y moleculares complejos. Las estrellas AGB son importantes
Domingo Aníbal
García Hernández