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000001885 005__ 20160701171654.0
000001885 0247_ $$2DOI$$a10.1086/174333
000001885 037__ $$aASTROimport-42
000001885 100__ $$aJohansson, S.
000001885 245__ $$aAnalysis of the 3d64s(6D)4f-5g supermultiplet of Fe I in laboratory and solar infrared spectra
000001885 260__ $$c1994
000001885 520__ $$aThe combined laboratory and solar analysis of the highly excited subconfigurations 3d64s(6D)4f and 3d64s(6D)5g of Fe I has allowed us to classify 87 lines of the 4f-5g supermultiplet in the spectral region 2545-2585 per cm. The level structure of these JK-coupled configurations is predicted by semiempirical calculations and the quardrupolic approximation. Semiempirical gf-values have been calculated and are compared to gf-values derived from the solar spectrum. The solar analysis has shown that these lines, which should be much less sensitive than lower excitation lines to departures from Local Thermal Equilibrium (LTE) and to temperature uncertanties, lead to a solar abundance of iron which is consistent with the meteoritic value (AFe = 7.51). 
000001885 700__ $$a Nave, G.
000001885 700__ $$a Geller, M.
000001885 700__ $$a Sauval, A. J.
000001885 700__ $$a Grevesse, N.
000001885 700__ $$a Schoenfeld, W. G.
000001885 700__ $$a Change, E. S.
000001885 700__ $$a Farmer, C. B.
000001885 773__ $$c419-426$$pThe Astrophysical Journal$$v429$$y1994
000001885 85642 $$ahttp://esoads.eso.org/abs/1994ApJ...429..419J
000001885 905__ $$apublished in
000001885 980__ $$aREFERD