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

Astronomy and Astrophysics

Volumn 495, Issue 2, 2009, Pages 655-661

  Warmbier, R ^a   Schneider, R ^a   Sharma, A R ^b   Braams, B J ^b   Bowman, J M ^b   Hauschildt, P H ^c  

^a MAX PLANCK INSTITUT FÜR PLASMAPHYSIK   (Germany)

^b EMORY UNIVERSITY   (United States)

^c UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Molecular data; Radiative transfer

Indexed keywords

APPLICATIONS; ASTROPHYSICS; ELECTRONIC STRUCTURE; METHANE; POTENTIAL ENERGY; RADIATIVE TRANSFER;

AB INITIO MODELING; AB-INITIO; AB-INITIO ELECTRONIC STRUCTURE CALCULATIONS; ASTROPHYSICAL APPLICATIONS; COMPLETE SETS; DIPOLE TRANSITIONS; EINSTEIN COEFFICIENTS; EMISSION SPECTRUMS; HITRAN DATABASE; HYPER-SURFACES; INFRARED SPECTROSCOPIC; IR SPECTRUM; LINE POSITIONS; LINE STRENGTHS; MODEL ATMOSPHERES; MOLECULAR DATA; MULTI MODES; POLYATOMIC MOLECULES; RO-VIBRATIONAL ENERGIES; SPECTROSCOPIC DATABASE; STATE ENERGIES; SYNTHETIC SPECTRUMS; WAVELENGTH REGIONS;

EMISSION SPECTROSCOPY;

EID: 61349190294     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810983     Document Type: Article

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