Table 2
Measured line fluxes (F) and extinction corrected line intensities (I) of HaTr 5, together with synthetic line intensities.
Line | ƒ(λ) | SAAO 2014 | SAAO 2024 | Shara et al. (2017) | Model | |||
---|---|---|---|---|---|---|---|---|
F/F(Hα) | I / I (Hα) | F/F(Hα) | I/I(Hα) | F/F(Hα) | I/I(Hα) | I/I(Hα) | ||
[O II] 3726 | +0.26 | … | … | 0.55±0.19: | 1.68 : | … | … | 1.02 |
Hδ 4101 | +0.18 | … | … | … | … | 0.03 | 0.08 | 0.09 |
Hγ 4340 | +0.14 | … | … | … | … | 0.05 | 0.12 | 0.17 |
He II 4686 | +0.05 | … | … | … | … | 0.017 | 0.035 | 0.02 |
Hβ 4861 | 0.00 | 0.21 ±0.07 : | 0.40: | 0.18±0.04 | 0.34 | 0.19 | 0.36 | 0.36 |
[O III] 5007 | −0.03 | … | … | 0.11±0.02 | 0.20 | 0.13 | 0.23 | 0.22 |
[N II] 5755 | −0.21 | … | … | … | … | 0.015 | 0.02 | 0.01 |
He I 5876 | −0.23 | … | … | … | … | 0.03 | 0.02 | 0.01 |
[O I] 6300 | −0.30 | … | … | 0.61±0.02: | 0.66 : | 0.17 | 0.19 | 0.10 |
[O I] 6363 | −0.30 | … | … | 0.15±0.02: | 0.16 : | 0.06 | 0.07 | 0.03 |
[N II] 6548 | −0.34 | 0.26±0.06 | 0.26 | 0.25±0.02 | 0.25 | 0.35 | 0.36 | 0.31 |
Hα 6563 | −0.34 | 1.00±0.06 | 1.00 | 1.00±0.02 | 1.00 | 1.00 | 1.00 | 1.00 |
[N II] 6584 | −0.34 | 1.14±0.07 | 1.14 | 0.81±0.02 | 0.81 | 1.19 | 1.22 | 0.92 |
[S II] 6716 | −0.36 | 0.55±0.06 | 0.53 | 0.37±0.02 | 0.36 | 0.30 | 0.30 | 0.33 |
[S II] 6731 | −0.36 | 0.49±0.06 | 0.47 | 0.26±0.02 | 0.25 | 0.22 | 0.22 | 0.24 |
F (Hα)a | 2.0 × 10−14 | 3.1 × 10−14 | … | … | ||||
SB(Hα)a | 1.0 × 10−16 | 2.0 × 10−16 | 1.3 × 10−16 | 3.0 × 10−16 |
Notes. The line fluxes and intensities are relative to Hα (=1.0). They correspond to observations obtained at SAAO on 2014 and 2024, and those from Shara et al. (2017), while the line intensity predictions have been derived from a Cloudy photoionization model. The observed Hα flux F(Hα) and surface brightness S B(Hα) are given in units of erg cm−2 s−1 and erg cm−2 s−1 arcsec−2, respectively. Line fluxes and intensities affected by large uncertainties are denoted by a “:” sign.
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