Ab initio modeling of molecular IR spectra of astrophysical interest: 
Application to CH4

Warmbier, R.; Schneider, R.; Sharma, A. R.; Braams, B. J.; Bowman, J. M.; Hauschildt, P. H.

doi:10.1051/0004-6361:200810983

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Ab initio modeling of molecular IR spectra of astrophysical interest: Application to CH₄

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Warmbier, R.
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;
Helmholtz Junior Research Group 'Computational Material Science' (Junior Research Group HGF-Greifswald), Max Planck Institute for Plasma Physics, Max Planck Society;

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Schneider, R.
Helmholtz Junior Research Group 'Computational Material Science' (Junior Research Group HFG-Greifswald), Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Theory (ST), Max Planck Institute for Plasma Physics, Max Planck Society;

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Warmbier, R., Schneider, R., Sharma, A. R., Braams, B. J., Bowman, J. M., & Hauschildt, P. H. (2009). Ab initio modeling of molecular IR spectra of astrophysical interest: Application to CH₄. Astronomy & Astrophysics, 495, 655-661. doi:10.1051/0004-6361:200810983.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0026-F57F-5

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