Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules

The vibronic (vibration-electronic) transition probability parameters such as Franck-Condon (FC) factors and r-centroids of diatomic molecular species could be useful in the identification of molecular bands and in the estimation of relative abundance of the emitted species in astrophysical sources....

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Main Authors: Shanmugavel R., Bagare S.P., Rajamanickam N.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2006-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2006/1450-698X0673083S.pdf
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author Shanmugavel R.
Bagare S.P.
Rajamanickam N.
author_facet Shanmugavel R.
Bagare S.P.
Rajamanickam N.
author_sort Shanmugavel R.
collection DOAJ
description The vibronic (vibration-electronic) transition probability parameters such as Franck-Condon (FC) factors and r-centroids of diatomic molecular species could be useful in the identification of molecular bands and in the estimation of relative abundance of the emitted species in astrophysical sources. In this study, they have been evaluated for the electronic transitions A2Πr-X2Σ+, B2Πr-X2Σ+ and C2Σ+ - X2Σ+ systems of BeH, A2Πr - X2Σ and C2Σ+ - X2Σ+ system of BeD and A2Πr - X2Σ+ system of BeT molecules using a suitable potential.
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spelling doaj.art-8e67642c92bb4349b93c1f08ecb184922022-12-21T22:25:03ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892006-01-012006173838710.2298/SAJ0673083S1450-698X0673083SAstrophysically useful parameters for certain band systems of BeH, BeD and BeT moleculesShanmugavel R.0Bagare S.P.1Rajamanickam N.2Physics Research Centre, V.H.N.S.N College, VirudhunagarIndian Institute of Astrophysics, Kodaikanal and BangalorePhysics Research Centre, V.H.N.S.N College, VirudhunagarThe vibronic (vibration-electronic) transition probability parameters such as Franck-Condon (FC) factors and r-centroids of diatomic molecular species could be useful in the identification of molecular bands and in the estimation of relative abundance of the emitted species in astrophysical sources. In this study, they have been evaluated for the electronic transitions A2Πr-X2Σ+, B2Πr-X2Σ+ and C2Σ+ - X2Σ+ systems of BeH, A2Πr - X2Σ and C2Σ+ - X2Σ+ system of BeD and A2Πr - X2Σ+ system of BeT molecules using a suitable potential.http://www.doiserbia.nb.rs/img/doi/1450-698X/2006/1450-698X0673083S.pdfmolecular datamethods: numericalsun: abundances
spellingShingle Shanmugavel R.
Bagare S.P.
Rajamanickam N.
Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
Serbian Astronomical Journal
molecular data
methods: numerical
sun: abundances
title Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
title_full Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
title_fullStr Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
title_full_unstemmed Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
title_short Astrophysically useful parameters for certain band systems of BeH, BeD and BeT molecules
title_sort astrophysically useful parameters for certain band systems of beh bed and bet molecules
topic molecular data
methods: numerical
sun: abundances
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2006/1450-698X0673083S.pdf
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