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) Ion . | EW(λ)a . | FWHM(λ)a . | RV . |
---|---|---|---|
. | (Å) . | (Å) . | ( km s−1) . |
3889 He ii + H8 | 1.35 ± 0.13 | 7.37 ± 0.16 | 311 ± 40 |
3968 He ii + H7 | 1.73 ± 0.17 | 8.32 ± 0.11 | 271 ± 11 |
4026 He ii | 0.56 ± 0.11 | 5.88 ± 0.15 | 353 ± 8 |
4100 He ii + Hδ | 1.67 ± 0.16 | 8.09 ± 0.14 | 285 ± 6 |
4144 He i | 0.05 ± 0.03 | 4.86 ± 0.35 | 307 ± 50 |
4200 He ii | 0.47 ± 0.11 | 5.82 ± 0.12 | 317 ± 8 |
4339 He ii + Hγ | 1.49 ± 0.15 | 7.81 ± 0.11 | 268 ± 6 |
4388 He i | 0.14 ± 0.09 | 5.08 ± 0.35 | 361 ± 35 |
4471 He i | 0.35 ± 0.08 | 4.12 ± 0.11 | 315 ± 6 |
4542 He ii | 0.62 ± 0.12 | 6.81 ± 0.18 | 266 ± 8 |
4604 N v | −2.50 ± 0.28 | 13.73 ± 0.51 | 192 ± 8 |
4620 N v | −1.50 ± 0.20 | 10.50 ± 2.00 | 219 ± 11 |
4686 He ii | 0.02 ± 0.03* | 3.28 ± 0.21* | 282 ± 25 |
4686 He ii | −16.37 ± 0.68* | 31.10 ± 0.21* | 280 ± 15 |
4859 He ii + Hβ | 1.14 ± 0.14* | 7.09 ± 0.15* | 244 ± 10 |
4859 He ii + Hβ | −1.52 ± 0.52* | 28.87 ± 4.09* | 146 ± 50 |
4922 He i | 0.11 ± 0.06 | 3.43 ± 0.28 | 306 ± 20 |
4944 N v | −0.50 ± 0.13 | 8.77 ± 0.43 | 175 ± 21 |
5412 He ii | 0.26 ± 0.07* | 5.36 ± 0.26* | 261 ± 10 |
5412 He ii | −2.41 ± 0.83* | 54.91 ± 2.10* | 270 ± 14 |
5592 O iii | 0.11 ± 0.05 | 4.40 ± 0.21 | 305 ± 14 |
5876 He i | 0.50 ± 0.07 | 4.64 ± 0.10 | 313 ± 21 |
6560 He ii + Hα | 0.56 ± 0.07* | 5.08 ± 0.15* | 211 ± 20 |
6563 He ii + Hα | −12.66 ± 0.86* | 47.58 ± 0.79* | 177 ± 15 |
6678 He i | 0.17 ± 0.05 | 4.66 ± 0.30 | 302 ± 9 |
λ0(Å) Ion . | EW(λ)a . | FWHM(λ)a . | RV . |
---|---|---|---|
. | (Å) . | (Å) . | ( km s−1) . |
3889 He ii + H8 | 1.35 ± 0.13 | 7.37 ± 0.16 | 311 ± 40 |
3968 He ii + H7 | 1.73 ± 0.17 | 8.32 ± 0.11 | 271 ± 11 |
4026 He ii | 0.56 ± 0.11 | 5.88 ± 0.15 | 353 ± 8 |
4100 He ii + Hδ | 1.67 ± 0.16 | 8.09 ± 0.14 | 285 ± 6 |
4144 He i | 0.05 ± 0.03 | 4.86 ± 0.35 | 307 ± 50 |
4200 He ii | 0.47 ± 0.11 | 5.82 ± 0.12 | 317 ± 8 |
4339 He ii + Hγ | 1.49 ± 0.15 | 7.81 ± 0.11 | 268 ± 6 |
4388 He i | 0.14 ± 0.09 | 5.08 ± 0.35 | 361 ± 35 |
4471 He i | 0.35 ± 0.08 | 4.12 ± 0.11 | 315 ± 6 |
4542 He ii | 0.62 ± 0.12 | 6.81 ± 0.18 | 266 ± 8 |
4604 N v | −2.50 ± 0.28 | 13.73 ± 0.51 | 192 ± 8 |
4620 N v | −1.50 ± 0.20 | 10.50 ± 2.00 | 219 ± 11 |
4686 He ii | 0.02 ± 0.03* | 3.28 ± 0.21* | 282 ± 25 |
4686 He ii | −16.37 ± 0.68* | 31.10 ± 0.21* | 280 ± 15 |
4859 He ii + Hβ | 1.14 ± 0.14* | 7.09 ± 0.15* | 244 ± 10 |
4859 He ii + Hβ | −1.52 ± 0.52* | 28.87 ± 4.09* | 146 ± 50 |
4922 He i | 0.11 ± 0.06 | 3.43 ± 0.28 | 306 ± 20 |
4944 N v | −0.50 ± 0.13 | 8.77 ± 0.43 | 175 ± 21 |
5412 He ii | 0.26 ± 0.07* | 5.36 ± 0.26* | 261 ± 10 |
5412 He ii | −2.41 ± 0.83* | 54.91 ± 2.10* | 270 ± 14 |
5592 O iii | 0.11 ± 0.05 | 4.40 ± 0.21 | 305 ± 14 |
5876 He i | 0.50 ± 0.07 | 4.64 ± 0.10 | 313 ± 21 |
6560 He ii + Hα | 0.56 ± 0.07* | 5.08 ± 0.15* | 211 ± 20 |
6563 He ii + Hα | −12.66 ± 0.86* | 47.58 ± 0.79* | 177 ± 15 |
6678 He i | 0.17 ± 0.05 | 4.66 ± 0.30 | 302 ± 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).
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) Ion . | EW(λ)a . | FWHM(λ)a . | RV . |
---|---|---|---|
. | (Å) . | (Å) . | ( km s−1) . |
3889 He ii + H8 | 1.35 ± 0.13 | 7.37 ± 0.16 | 311 ± 40 |
3968 He ii + H7 | 1.73 ± 0.17 | 8.32 ± 0.11 | 271 ± 11 |
4026 He ii | 0.56 ± 0.11 | 5.88 ± 0.15 | 353 ± 8 |
4100 He ii + Hδ | 1.67 ± 0.16 | 8.09 ± 0.14 | 285 ± 6 |
4144 He i | 0.05 ± 0.03 | 4.86 ± 0.35 | 307 ± 50 |
4200 He ii | 0.47 ± 0.11 | 5.82 ± 0.12 | 317 ± 8 |
4339 He ii + Hγ | 1.49 ± 0.15 | 7.81 ± 0.11 | 268 ± 6 |
4388 He i | 0.14 ± 0.09 | 5.08 ± 0.35 | 361 ± 35 |
4471 He i | 0.35 ± 0.08 | 4.12 ± 0.11 | 315 ± 6 |
4542 He ii | 0.62 ± 0.12 | 6.81 ± 0.18 | 266 ± 8 |
4604 N v | −2.50 ± 0.28 | 13.73 ± 0.51 | 192 ± 8 |
4620 N v | −1.50 ± 0.20 | 10.50 ± 2.00 | 219 ± 11 |
4686 He ii | 0.02 ± 0.03* | 3.28 ± 0.21* | 282 ± 25 |
4686 He ii | −16.37 ± 0.68* | 31.10 ± 0.21* | 280 ± 15 |
4859 He ii + Hβ | 1.14 ± 0.14* | 7.09 ± 0.15* | 244 ± 10 |
4859 He ii + Hβ | −1.52 ± 0.52* | 28.87 ± 4.09* | 146 ± 50 |
4922 He i | 0.11 ± 0.06 | 3.43 ± 0.28 | 306 ± 20 |
4944 N v | −0.50 ± 0.13 | 8.77 ± 0.43 | 175 ± 21 |
5412 He ii | 0.26 ± 0.07* | 5.36 ± 0.26* | 261 ± 10 |
5412 He ii | −2.41 ± 0.83* | 54.91 ± 2.10* | 270 ± 14 |
5592 O iii | 0.11 ± 0.05 | 4.40 ± 0.21 | 305 ± 14 |
5876 He i | 0.50 ± 0.07 | 4.64 ± 0.10 | 313 ± 21 |
6560 He ii + Hα | 0.56 ± 0.07* | 5.08 ± 0.15* | 211 ± 20 |
6563 He ii + Hα | −12.66 ± 0.86* | 47.58 ± 0.79* | 177 ± 15 |
6678 He i | 0.17 ± 0.05 | 4.66 ± 0.30 | 302 ± 9 |
λ0(Å) Ion . | EW(λ)a . | FWHM(λ)a . | RV . |
---|---|---|---|
. | (Å) . | (Å) . | ( km s−1) . |
3889 He ii + H8 | 1.35 ± 0.13 | 7.37 ± 0.16 | 311 ± 40 |
3968 He ii + H7 | 1.73 ± 0.17 | 8.32 ± 0.11 | 271 ± 11 |
4026 He ii | 0.56 ± 0.11 | 5.88 ± 0.15 | 353 ± 8 |
4100 He ii + Hδ | 1.67 ± 0.16 | 8.09 ± 0.14 | 285 ± 6 |
4144 He i | 0.05 ± 0.03 | 4.86 ± 0.35 | 307 ± 50 |
4200 He ii | 0.47 ± 0.11 | 5.82 ± 0.12 | 317 ± 8 |
4339 He ii + Hγ | 1.49 ± 0.15 | 7.81 ± 0.11 | 268 ± 6 |
4388 He i | 0.14 ± 0.09 | 5.08 ± 0.35 | 361 ± 35 |
4471 He i | 0.35 ± 0.08 | 4.12 ± 0.11 | 315 ± 6 |
4542 He ii | 0.62 ± 0.12 | 6.81 ± 0.18 | 266 ± 8 |
4604 N v | −2.50 ± 0.28 | 13.73 ± 0.51 | 192 ± 8 |
4620 N v | −1.50 ± 0.20 | 10.50 ± 2.00 | 219 ± 11 |
4686 He ii | 0.02 ± 0.03* | 3.28 ± 0.21* | 282 ± 25 |
4686 He ii | −16.37 ± 0.68* | 31.10 ± 0.21* | 280 ± 15 |
4859 He ii + Hβ | 1.14 ± 0.14* | 7.09 ± 0.15* | 244 ± 10 |
4859 He ii + Hβ | −1.52 ± 0.52* | 28.87 ± 4.09* | 146 ± 50 |
4922 He i | 0.11 ± 0.06 | 3.43 ± 0.28 | 306 ± 20 |
4944 N v | −0.50 ± 0.13 | 8.77 ± 0.43 | 175 ± 21 |
5412 He ii | 0.26 ± 0.07* | 5.36 ± 0.26* | 261 ± 10 |
5412 He ii | −2.41 ± 0.83* | 54.91 ± 2.10* | 270 ± 14 |
5592 O iii | 0.11 ± 0.05 | 4.40 ± 0.21 | 305 ± 14 |
5876 He i | 0.50 ± 0.07 | 4.64 ± 0.10 | 313 ± 21 |
6560 He ii + Hα | 0.56 ± 0.07* | 5.08 ± 0.15* | 211 ± 20 |
6563 He ii + Hα | −12.66 ± 0.86* | 47.58 ± 0.79* | 177 ± 15 |
6678 He i | 0.17 ± 0.05 | 4.66 ± 0.30 | 302 ± 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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