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Table 1.
All emission lines measured in this study.
Atom/Ion | λ (Å) | Atom/Ion | λ (Å) |
---|---|---|---|
OII | 3726.03 | OIII* | 5006.84 |
OII* | 3728.73 | HeI | 5016.51 |
H9 | 3751.09 | NII | 5754.59 |
Hth | 3798.96 | HeI* | 5875.61 |
Ht | 3836.26 | OI* | 6300.30 |
NeIII | 3868.69 | SIII | 6312.06 |
NeIII | 3967.40 | OI | 6363.78 |
He | 3970.07 | NII | 6548.05 |
SII | 4068.60 | Ha* | 6562.82 |
SII | 4076.35 | NII | 6583.45 |
Hd* | 4101.73 | HeI | 6678.15 |
FeII | 4288.10 | HeI | 6680.05 |
Hg* | 4340.46 | SII | 6716.44 |
FeII | 4359.33 | SII | 6730.81 |
OIII | 4363.20 | ArIII* | 7135.67 |
FeIII | 4659.10 | OII | 7318.92 |
HeII | 4685.70 | OII | 7319.99 |
ArIV | 4713.00 | OII | 7329.67 |
Hb* | 4861.33 | OII | 7330.73 |
OIII | 4958.91 | TiII | 8448.36 |
HeI | 4987.44 | FeII | 8574.85 |
SIII* | 9068.61 |
Notes. Each box represents the wavelength range over which the spectra are modeled. The kinematics of the spectral lines are anchored to the most prominent line within each interval, indicated by a star symbol.
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