Identification of vibration-rotation lines of CH in the solar infrared spectrum

Details Identification of vibration-rotation lines of CH in the solar infrared spectrum Identification of vibration-rotation lines of CH in the solar infrared spectrum

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aexpr...1..153s&link_type=abstract

Astronomy Express (ISSN 0265-5365), vol. 1, June 1985, p. 153-158.

Astronomy and Astrophysics

Astronomy

2

Hydrocarbons, Infrared Spectra, Molecular Oscillations, Molecular Rotation, Solar Spectra, Stellar Spectrophotometry, Abundance, Carbon, Cool Stars, Dipole Moments, Fourier Transformation

Scientific paper

Transitions of the fundamental band of CH have recently been measured
with very high accuracy by Lubic and Amano (1984). The lines are shown
to be present in the solar infrared spectrum (2580 - 2940
cm-1). The role these lines could play in solar and stellar
spectroscopy is discussed.

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