000001907 001__ 1907
000001907 005__ 20160701171655.0
000001907 037__ $$aASTROimport-64
000001907 100__ $$aGrevesse, N.
000001907 245__ $$aVibration-rotation bands of CH in the solar infrared spectrum and the solar carbon abundance
000001907 260__ $$c1991
000001907 520__ $$aHigh resolution solar spectra obtained from the ATMOS Fourier Transform Spectrometer (Spacelab 3 flight on April 29-May 6, 1985) have made it possible to identify and measure a large number of lines of the vibration-rotation fundamental bands of the X2 Pi state of CH. From about 100 lines of the 1-0, 2-1, and 3-2 bands and adopting theoretical transition probabilities, a solar carbon abundance of 8.60 + or - 0.05 is derived. This value is compared with new results inferred from other carbon abundance indicators. The final recommended solar abundance of carbon is 8.60 + or - 0.05. 
000001907 700__ $$a Lambert, D. L.
000001907 700__ $$a Sauval, A. J.
000001907 700__ $$a van Dishoeck, E. F.
000001907 700__ $$a Farmer, C. B.
000001907 700__ $$a Norton, R. H.
000001907 773__ $$c488-495$$pAstronomy and Astrophysics$$v242$$y1991
000001907 85642 $$ahttp://esoads.eso.org/abs/1991A%26A...242..488G
000001907 905__ $$apublished in
000001907 980__ $$aREFERD