Astrophysically Useful Parameters for Some Vibronic Transitions of AlH and BH
- 6 December 2006
- journal article
- research article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 306 (4) , 231-234
- https://doi.org/10.1007/s10509-006-9261-2
Abstract
No abstract availableKeywords
This publication has 16 references indexed in Scilit:
- Identification of AlF Molecular Lines in Sunspot Umbral SpectraSolar Physics, 2006
- Precise Rest Frequencies for AlH and AlD ( X 1 + ): A Reassessment of the Aluminum Hyperfine StructureThe Astrophysical Journal, 2004
- Molecular parameters for D, E, F, and G-A band systems of the astrophysically significant molecule AlFAstrophysics and Space Science, 2004
- Franck–Condon factors and r-centroids for a number of band systems of the astrophysical molecule AlFAstroparticle Physics, 2003
- Emission Spectroscopy of the Triplet System of the BH RadicalJournal of Molecular Spectroscopy, 1996
- Molecular Spectra and Molecular StructurePublished by Springer Nature ,1979
- Abundances of Interstellar CH and CH^{+} RadicalsThe Astrophysical Journal, 1972
- The diatomic molecules BH, BN, and BO in sunspots and the solar abundance of boronSolar Physics, 1970
- Identification of Aluminum Hydride as the Emitter of Bright Lines Observed in χ Cygni Near Minimum LightPublications of the Astronomical Society of the Pacific, 1956
- Chemical Compounds in the Sun.The Astrophysical Journal, 1945