Oxygen lines in solar granulation - II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance

T. M. D. Pereira; M. Asplund; D. Kiselman

doi:10.1051/0004-6361/200912840

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Volume 508 / No 3 (December IV 2009)

A&A, 508 3 (2009) 1403-1416

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Table 5:

Molecular lines included in the 615.8 nm region.
Mol.	Wavelength	System	Band	$\log gf$	$E_{{\rm low}}$
	[nm]				[eV]
CN	615.7850	A-X	(7, 2)	-1.498	1.800
C $_{\rm 2}$	615.8106	$d^3\Pi_g-a^3\Pi_u$	(0, 2)	-1.652	0.508
CN	615.8109	A-X	(6, 1)	-2.140	1.093
CN	615.8223	A-X	(10, 4)	-1.613	2.066
CN	615.8522	A-X	(9, 4)	-1.959	1.062
CN	615.8796	A-X	(9, 4)	-1.924	1.088

Source LaTeX | All tables | In the text

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