RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules
Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09...
Ausführliche Beschreibung
Autor*in: |
Reddy, R.R. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1998 |
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Schlagwörter: |
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Anmerkung: |
© Kluwer Academic Publishers 1998 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 262(1998), 2 vom: Juni, Seite 223-240 |
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Übergeordnetes Werk: |
volume:262 ; year:1998 ; number:2 ; month:06 ; pages:223-240 |
Links: |
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DOI / URN: |
10.1023/A:1001848028629 |
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Katalog-ID: |
OLC2066216925 |
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520 | |a Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. | ||
650 | 4 | |a Potential Energy | |
650 | 4 | |a Dissociation Energy | |
650 | 4 | |a Energy Curve | |
650 | 4 | |a Electronic Ground State | |
650 | 4 | |a Potential Energy Curve | |
700 | 1 | |a Nazeer Ahammed, Y. |4 aut | |
700 | 1 | |a Rama Gopal, K. |4 aut | |
700 | 1 | |a Abdul Azeem, P. |4 aut | |
700 | 1 | |a Anjaneyulu, S. |4 aut | |
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10.1023/A:1001848028629 doi (DE-627)OLC2066216925 (DE-He213)A:1001848028629-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Reddy, R.R. verfasserin aut RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve Nazeer Ahammed, Y. aut Rama Gopal, K. aut Abdul Azeem, P. aut Anjaneyulu, S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 262(1998), 2 vom: Juni, Seite 223-240 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:262 year:1998 number:2 month:06 pages:223-240 https://doi.org/10.1023/A:1001848028629 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 262 1998 2 06 223-240 |
spelling |
10.1023/A:1001848028629 doi (DE-627)OLC2066216925 (DE-He213)A:1001848028629-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Reddy, R.R. verfasserin aut RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve Nazeer Ahammed, Y. aut Rama Gopal, K. aut Abdul Azeem, P. aut Anjaneyulu, S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 262(1998), 2 vom: Juni, Seite 223-240 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:262 year:1998 number:2 month:06 pages:223-240 https://doi.org/10.1023/A:1001848028629 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 262 1998 2 06 223-240 |
allfields_unstemmed |
10.1023/A:1001848028629 doi (DE-627)OLC2066216925 (DE-He213)A:1001848028629-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Reddy, R.R. verfasserin aut RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve Nazeer Ahammed, Y. aut Rama Gopal, K. aut Abdul Azeem, P. aut Anjaneyulu, S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 262(1998), 2 vom: Juni, Seite 223-240 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:262 year:1998 number:2 month:06 pages:223-240 https://doi.org/10.1023/A:1001848028629 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 262 1998 2 06 223-240 |
allfieldsGer |
10.1023/A:1001848028629 doi (DE-627)OLC2066216925 (DE-He213)A:1001848028629-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Reddy, R.R. verfasserin aut RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve Nazeer Ahammed, Y. aut Rama Gopal, K. aut Abdul Azeem, P. aut Anjaneyulu, S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 262(1998), 2 vom: Juni, Seite 223-240 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:262 year:1998 number:2 month:06 pages:223-240 https://doi.org/10.1023/A:1001848028629 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 262 1998 2 06 223-240 |
allfieldsSound |
10.1023/A:1001848028629 doi (DE-627)OLC2066216925 (DE-He213)A:1001848028629-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Reddy, R.R. verfasserin aut RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules 1998 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1998 Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve Nazeer Ahammed, Y. aut Rama Gopal, K. aut Abdul Azeem, P. aut Anjaneyulu, S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 262(1998), 2 vom: Juni, Seite 223-240 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:262 year:1998 number:2 month:06 pages:223-240 https://doi.org/10.1023/A:1001848028629 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 262 1998 2 06 223-240 |
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English |
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Enthalten in Astrophysics and space science 262(1998), 2 vom: Juni, Seite 223-240 volume:262 year:1998 number:2 month:06 pages:223-240 |
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Enthalten in Astrophysics and space science 262(1998), 2 vom: Juni, Seite 223-240 volume:262 year:1998 number:2 month:06 pages:223-240 |
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Potential Energy Dissociation Energy Energy Curve Electronic Ground State Potential Energy Curve |
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The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. 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RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules |
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RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules |
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rkrv potential energy curves, dissociation energies, γ-centroids and franck-condon factors of yo, cro, bn, sco, sio and alo molecules |
title_auth |
RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules |
abstract |
Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. © Kluwer Academic Publishers 1998 |
abstractGer |
Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. © Kluwer Academic Publishers 1998 |
abstract_unstemmed |
Abstract The potential energy curves for the electronic ground states of astrophysically important YO, CrO, BN, ScO, SiO and AlO molecules are constructed techniques using the five-parameter Hulburt-Hirschfelder function. The estimated dissociation energies are 7.235±0.15, 4.337 ± 0.09, 3.917 ± 0.09, 6.899 ± 0.14, 8.181 ± 0.17 and 5.202 ± 0.11 eV for YO, CrO, BN, ScO, SiO and AlO, respectively. The estimated $ D_{0} $ values are in reasonably good agreement with literature values. The r-Centroids and Franck-Condon factors for the bands of $ B^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ of YO, $ B^{5} $ Π −$ X^{5} $ Π> of CrO, $ A^{3} $ Π − $ X^{3} $ Π of BN, $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of ScO, $ E^{1} $ $ Σ^{+} $ − $ X^{1} $ $ Σ^{+} $ of SiO and $ D^{2} $ $ Σ^{+} $ − $ X^{2} $ $ Σ^{+} $ and $ B^{2} $ $ Σ^{+} $ −$ X^{2} $ $ Σ^{+} $ of AlO molecules have been determined. The Franck-Condon factors are evaluated by the approximate analytical method of Jarmain and Fraser. The absence of the bands in these systems is explained. © Kluwer Academic Publishers 1998 |
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RKRV Potential Energy Curves, Dissociation Energies, γ-Centroids And Franck-Condon Factors Of YO, CrO, BN, ScO, SiO And AlO Molecules |
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