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Table 3.

Noticeable emission lines in the NIR.

Ion Rest wavelength Velocity Dopplershift (a) Comment
(micron) (km s−1) (km s−1)
H I 1.282 1084 −164 Pβ, mainly red side
H I 2.166 1038 −117 Brγ, mainly red side
H2 1.747 971 −14 Potentially
H2 2.121 Not strong, only red side, maybe also 1.957 and 2.033
He I 1.012 1107 −141
He I 1.083 1189 −74 Several components
He I 1.279 968 −111 Only red reliable
He I 2.059 1070 −167 Red side strong
[S II] 1.032 731 712 Two components of this quadruple?
[S II] 1.037 724 247
[Fe II] 1.189 1066 −154
[Fe II] 1.257 1175 −172 Strong
[Fe II] 1.295 Weak, only red side
[Fe II] 1.321 1180 −190
[Fe II] 1.533 1057 −174 Red side clear
[Fe II] 1.600 1066 −210 Red side very clear
[Fe II] 1.644 1189 −170 Strong
[Fe II] 1.677 Only red side
[Fe II] 1.811 1015 −400 Weaker
[P II] 1.189 1060 493 Phosphorus, maybe also 1.147

Notes.

(a)

Most lines come both blue and redshifted. The velocities tabulated are ± the velocity offset from center, and the Dopplershift is a measure of that central wavelength versus the given rest wavelength. These were measured on the 2D frame of OB6. There also seems to be some lines we did not identify, for example at wavelengths 1.38, 1.82, 1.88, 1.95 microns.

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