Table 3.

EWs, FWHMs and RVs of main lines in the spectrum of the new WR star BAT99 3a (star 1). For EWs and RVs, we give their mean values derived from both Gemini spectra, while for measurements of FWHMs, we used the second spectrum alone owing to its better quality.

λ0(Å) IonEW(λ)aFWHM(λ)aRV
(Å)(Å)( km s−1)
3889 He ii + H8 1.35 ± 0.137.37 ± 0.16311 ± 40
3968 He ii + H71.73 ± 0.178.32 ± 0.11271 ± 11
4026 He ii0.56 ± 0.115.88 ± 0.15353 ± 8
4100 He ii + Hδ1.67 ± 0.168.09 ± 0.14285 ± 6
4144 He i0.05 ± 0.034.86 ± 0.35307 ± 50
4200 He ii0.47 ± 0.115.82 ± 0.12317 ± 8
4339 He ii + Hγ1.49 ± 0.157.81 ± 0.11268 ± 6
4388 He i0.14 ± 0.095.08 ± 0.35361 ± 35
4471 He i0.35 ± 0.084.12 ± 0.11315 ± 6
4542 He ii0.62 ± 0.126.81 ± 0.18266 ± 8
4604 N v−2.50 ± 0.2813.73 ± 0.51192 ± 8
4620 N v−1.50 ± 0.2010.50 ± 2.00219 ± 11
4686 He ii0.02 ± 0.03*3.28 ± 0.21*282 ± 25
4686 He ii−16.37 ± 0.68*31.10 ± 0.21*280 ± 15
4859 He ii + Hβ1.14 ± 0.14*7.09 ± 0.15*244 ± 10
4859 He ii + Hβ−1.52 ± 0.52*28.87 ± 4.09*146 ± 50
4922 He i0.11 ± 0.063.43 ± 0.28306 ± 20
4944 N v−0.50 ± 0.138.77 ± 0.43175 ± 21
5412 He ii0.26 ± 0.07*5.36 ± 0.26*261 ± 10
5412 He ii−2.41 ± 0.83*54.91 ± 2.10*270 ± 14
5592 O iii0.11 ± 0.054.40 ± 0.21305 ± 14
5876 He i0.50 ± 0.074.64 ± 0.10313 ± 21
6560 He ii + Hα0.56 ± 0.07*5.08 ± 0.15*211 ± 20
6563 He ii + Hα−12.66 ± 0.86*47.58 ± 0.79*177 ± 15
6678 He i0.17 ± 0.054.66 ± 0.30302 ± 9
λ0(Å) IonEW(λ)aFWHM(λ)aRV
(Å)(Å)( km s−1)
3889 He ii + H8 1.35 ± 0.137.37 ± 0.16311 ± 40
3968 He ii + H71.73 ± 0.178.32 ± 0.11271 ± 11
4026 He ii0.56 ± 0.115.88 ± 0.15353 ± 8
4100 He ii + Hδ1.67 ± 0.168.09 ± 0.14285 ± 6
4144 He i0.05 ± 0.034.86 ± 0.35307 ± 50
4200 He ii0.47 ± 0.115.82 ± 0.12317 ± 8
4339 He ii + Hγ1.49 ± 0.157.81 ± 0.11268 ± 6
4388 He i0.14 ± 0.095.08 ± 0.35361 ± 35
4471 He i0.35 ± 0.084.12 ± 0.11315 ± 6
4542 He ii0.62 ± 0.126.81 ± 0.18266 ± 8
4604 N v−2.50 ± 0.2813.73 ± 0.51192 ± 8
4620 N v−1.50 ± 0.2010.50 ± 2.00219 ± 11
4686 He ii0.02 ± 0.03*3.28 ± 0.21*282 ± 25
4686 He ii−16.37 ± 0.68*31.10 ± 0.21*280 ± 15
4859 He ii + Hβ1.14 ± 0.14*7.09 ± 0.15*244 ± 10
4859 He ii + Hβ−1.52 ± 0.52*28.87 ± 4.09*146 ± 50
4922 He i0.11 ± 0.063.43 ± 0.28306 ± 20
4944 N v−0.50 ± 0.138.77 ± 0.43175 ± 21
5412 He ii0.26 ± 0.07*5.36 ± 0.26*261 ± 10
5412 He ii−2.41 ± 0.83*54.91 ± 2.10*270 ± 14
5592 O iii0.11 ± 0.054.40 ± 0.21305 ± 14
5876 He i0.50 ± 0.074.64 ± 0.10313 ± 21
6560 He ii + Hα0.56 ± 0.07*5.08 ± 0.15*211 ± 20
6563 He ii + Hα−12.66 ± 0.86*47.58 ± 0.79*177 ± 15
6678 He i0.17 ± 0.054.66 ± 0.30302 ± 9

aNote that some of the starred EWs and FWHMs are significantly affected because of the binary nature of BAT99 3a. The negative (positive) EWs correspond to emission (absorption) lines originating from the WR (O) component of BAT99 3a (see the text for details).

Table 3.

EWs, FWHMs and RVs of main lines in the spectrum of the new WR star BAT99 3a (star 1). For EWs and RVs, we give their mean values derived from both Gemini spectra, while for measurements of FWHMs, we used the second spectrum alone owing to its better quality.

λ0(Å) IonEW(λ)aFWHM(λ)aRV
(Å)(Å)( km s−1)
3889 He ii + H8 1.35 ± 0.137.37 ± 0.16311 ± 40
3968 He ii + H71.73 ± 0.178.32 ± 0.11271 ± 11
4026 He ii0.56 ± 0.115.88 ± 0.15353 ± 8
4100 He ii + Hδ1.67 ± 0.168.09 ± 0.14285 ± 6
4144 He i0.05 ± 0.034.86 ± 0.35307 ± 50
4200 He ii0.47 ± 0.115.82 ± 0.12317 ± 8
4339 He ii + Hγ1.49 ± 0.157.81 ± 0.11268 ± 6
4388 He i0.14 ± 0.095.08 ± 0.35361 ± 35
4471 He i0.35 ± 0.084.12 ± 0.11315 ± 6
4542 He ii0.62 ± 0.126.81 ± 0.18266 ± 8
4604 N v−2.50 ± 0.2813.73 ± 0.51192 ± 8
4620 N v−1.50 ± 0.2010.50 ± 2.00219 ± 11
4686 He ii0.02 ± 0.03*3.28 ± 0.21*282 ± 25
4686 He ii−16.37 ± 0.68*31.10 ± 0.21*280 ± 15
4859 He ii + Hβ1.14 ± 0.14*7.09 ± 0.15*244 ± 10
4859 He ii + Hβ−1.52 ± 0.52*28.87 ± 4.09*146 ± 50
4922 He i0.11 ± 0.063.43 ± 0.28306 ± 20
4944 N v−0.50 ± 0.138.77 ± 0.43175 ± 21
5412 He ii0.26 ± 0.07*5.36 ± 0.26*261 ± 10
5412 He ii−2.41 ± 0.83*54.91 ± 2.10*270 ± 14
5592 O iii0.11 ± 0.054.40 ± 0.21305 ± 14
5876 He i0.50 ± 0.074.64 ± 0.10313 ± 21
6560 He ii + Hα0.56 ± 0.07*5.08 ± 0.15*211 ± 20
6563 He ii + Hα−12.66 ± 0.86*47.58 ± 0.79*177 ± 15
6678 He i0.17 ± 0.054.66 ± 0.30302 ± 9
λ0(Å) IonEW(λ)aFWHM(λ)aRV
(Å)(Å)( km s−1)
3889 He ii + H8 1.35 ± 0.137.37 ± 0.16311 ± 40
3968 He ii + H71.73 ± 0.178.32 ± 0.11271 ± 11
4026 He ii0.56 ± 0.115.88 ± 0.15353 ± 8
4100 He ii + Hδ1.67 ± 0.168.09 ± 0.14285 ± 6
4144 He i0.05 ± 0.034.86 ± 0.35307 ± 50
4200 He ii0.47 ± 0.115.82 ± 0.12317 ± 8
4339 He ii + Hγ1.49 ± 0.157.81 ± 0.11268 ± 6
4388 He i0.14 ± 0.095.08 ± 0.35361 ± 35
4471 He i0.35 ± 0.084.12 ± 0.11315 ± 6
4542 He ii0.62 ± 0.126.81 ± 0.18266 ± 8
4604 N v−2.50 ± 0.2813.73 ± 0.51192 ± 8
4620 N v−1.50 ± 0.2010.50 ± 2.00219 ± 11
4686 He ii0.02 ± 0.03*3.28 ± 0.21*282 ± 25
4686 He ii−16.37 ± 0.68*31.10 ± 0.21*280 ± 15
4859 He ii + Hβ1.14 ± 0.14*7.09 ± 0.15*244 ± 10
4859 He ii + Hβ−1.52 ± 0.52*28.87 ± 4.09*146 ± 50
4922 He i0.11 ± 0.063.43 ± 0.28306 ± 20
4944 N v−0.50 ± 0.138.77 ± 0.43175 ± 21
5412 He ii0.26 ± 0.07*5.36 ± 0.26*261 ± 10
5412 He ii−2.41 ± 0.83*54.91 ± 2.10*270 ± 14
5592 O iii0.11 ± 0.054.40 ± 0.21305 ± 14
5876 He i0.50 ± 0.074.64 ± 0.10313 ± 21
6560 He ii + Hα0.56 ± 0.07*5.08 ± 0.15*211 ± 20
6563 He ii + Hα−12.66 ± 0.86*47.58 ± 0.79*177 ± 15
6678 He i0.17 ± 0.054.66 ± 0.30302 ± 9

aNote that some of the starred EWs and FWHMs are significantly affected because of the binary nature of BAT99 3a. The negative (positive) EWs correspond to emission (absorption) lines originating from the WR (O) component of BAT99 3a (see the text for details).

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