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000001878 0247_ $$2DOI$$a10.1006/jmsp.1995.0018
000001878 037__ $$aASTROimport-35
000001878 100__ $$aMelen, F.
000001878 245__ $$aA new analysis of the OH radical spectrum from solar infrared observations.
000001878 260__ $$c1995
000001878 520__ $$aThe solar spectrum offered the opportunity to discover OH lines with high rotational quantum numbers, which do not appear on laboratory spectra. On solar absorption spectra, the authors have identified about 580 lines, among which about 400 were observed for the first time. They belong to pure rotational transitions in the ground state (υ = 0→3; Jmax″= 48.5), as well as to the (1-0), (2-1), and (3-2) vibration-rotation bands (Jmax″= 32.5). Previous pure rotation, vibration-rotation, and Λ-doubling data sets related to the υ = 0 up to 3 levels were fitted simultaneously together with this new set of data, in order to obtain a very complete and accurate set of molecular constants for the X2Π ground state. 
000001878 700__ $$a Sauval, A. J.
000001878 700__ $$a Grevesse, N.
000001878 700__ $$a Farmer, C. B.
000001878 700__ $$a Servais, C.
000001878 700__ $$a Delbouille, L.
000001878 700__ $$a Roland, G.
000001878 773__ $$c490-509$$pJournal of Molecular Spectroscopy$$v174$$y1995
000001878 85642 $$ahttp://esoads.eso.org/abs/1995JMoSp.174..490M
000001878 905__ $$apublished in
000001878 980__ $$aREFERD