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Table 2

Carbon lines identified in the FUSE spectra of at least one of our program stars.

Wavelength Ion Transition

977.02 C iii 2s21S − 2s2p 1Po
1001.99: C iii 3p 1Po − 6d 1D
1016.34, 1016.40, 1016.53 C iii
1125.63–1125.68 C iii
1139.90 C iii 3p 1Po − 5d 1D
1165.62–1165.88a C iii 3p 3Po − 5d 3D
1174.93, 1175.26, 1175.59,
 1175.71, 1175.99, 1176.37 C iii 2s2p 3Po − 2p23P
948.09, 948.21 C iv 3s − 4p
1048.98c, 1049.02c C iv 4d − 11f
1050.04c C iv 4f − 11g
1060.59, 1060.74 C iv 4p − 10d
1066.63, 1066.78b C iv 4p − 10s
1097.32, 1097.34 C iv 4s − 8p
1107.59, 1107.93 C iv 3p − 4d
1108.89:, 1109.06: C iv 4p − 9d
1118.25:, 1118.41: C iv 4p − 9s
1134.25, 1134.30 C iv 4d − 9f
1135.50 C iv 4f − 9g
1135.64 C iv 4f − 9d
1136.63, 1136.68 C iv 4d − 9p
1168.85, 1168.99 C iv 3d − 4f
1184.59, 1184.77 C iv 4p − 8d

Notes. Wavelengths in Å. Colons denote uncertain identifications of very weak or blended lines;

(a)

blend Fe vi;

(b)

blend Si iv;

(c)

not included in model spectra.

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