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000001914 037__ $$aASTROimport-71
000001914 100__ $$aGrevesse, N.
000001914 245__ $$aIdentification of solar vibration-rotation lines of NH and the solar nitrogen abundance
000001914 260__ $$c1990
000001914 520__ $$aHigh resolution solar spectra obtained from the ATMOS Fourier Transform Spectrometer (Spacelab 3 flight on April 29 - May 6, 1985) made it possible to detect for the first time vibration-rotation lines of NH from the X3 Sigma(-) state near 3 microns. Using recent theoretical results for the transition probabilities of 23 selected measured lines of the 1-0 and 2-1 bands, a solar abundance of nitrogen of 8.06 + or - 0.07 is derived. This value is compared with the result derived from N I lines and agrees with the abundance obtained from the 3s-3p, 3p-3d and 3s-prime - 3p-prime transitions, A(N) = 8.00 + or - 0.09. The final recommended solar abundance of nitrogen is A(N) = 8.00 + or - 0.05. 
000001914 700__ $$a Lambert, D. L.
000001914 700__ $$a Sauval, A. J.
000001914 700__ $$a van Dishoeck, E. F.
000001914 700__ $$a Farmer, C. B.
000001914 700__ $$a Norton, R. H.
000001914 773__ $$c225-230$$pAstronomy and Astrophysics$$v232$$y1990
000001914 85642 $$ahttp://esoads.eso.org/abs/1990A%26A...232..225G
000001914 905__ $$apublished in
000001914 980__ $$aREFERD