Table 2: Line identifications and equivalent widths (EWs; given in Å) for the K band ($\sim $2-2.35 $\mu $m) spectra of AFGL 2298. Note that we have adopted the convention that emission lines are quoted as positive throughout the table. We estimate errors of $\pm $10 per cent for the UKIRT spectra and $\pm $20 per cent for the spectra from Campo Imperatore. Dates are given in month/year form for brevity; the exact dates of spectra are listed in Sect. 2.2. Note that within the observational uncertainties the EW measured from the 3 low resolution spectra taken between 2002 May-July are identical to one another (hence we only quote a mean value) while the values obtained from 2001 August (PC02) are identical to those obtained in 2001 June (and are also omitted for brevity).
Date 06/01 05/02 08/02
Transition   EW(Å)  
[Fe  II] (a45/2 - a2P3/2) 1.9 ? 5.0
He  I (2s1S - 2p1P0) 2.058 14.3 58 49.6
Fe  II (z4F3/2 - c4F3/2) 2.091 15.8 24 24.2
He  I (3p3P0 - 4s3S) 2.112 -0.8 8 6.3
+ He  I (3p1P0 - 4s1S) 2.113 bl bl bl
Fe  II (c4P03/2 - z4D05/2) 2.1177 2.1 ? bl
Mg  II (5s2S1/2 - 5p2P01/2) 2.138 5.2 13 6.9
Mg  II (5s2S1/2 - 5p2P01/2) 2.144 2.8 bl 4.7
He  I (4p3P - 7s3S) 2.15 -0.2 ? -
Br$\gamma$ 2.1661 31.0 90 81.6
He  I (4p1P - 7d1D) 2.185 1.5 - 1.5
Na  I (4p2 P03/2 - 4s2S1/2) 2.209 2.4 - -
+Na  I (4p2 P03/2 - 4s2S1/2) 2.206 bl - -
Fe  II (a2H11/2 - a2G9/2) 2.224 1.2 - 2.2
Fe  II (a4P1/2 - a2P3/2) 2.244 2.6 - 5.7


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