Table 6.

Ratios of near-IR diagnostic lines for newly identified WR stars from NTT/SOFI spectroscopy plus revised near-IR classifications for previously known stars. Line strengths/widths are provided for He ii 1.012 μm (2.189 μm in parenthesis) or C iv 1.736 μm (1.190 μm in parenthesis) for WN and WC stars, respectively.

IDWR1.01 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(P β/(He i 1.70/(Br γ/(He i+N iii 2.11/SpTSpT
km s−1He ii 1.01)He ii 1.16)He ii 1.69)He ii 2.19)N v 2.10)
B#13WR47-51000+0.08WN6−0.17(h)−0.55WN4−0.01(h)>0WN5–6WN6(h)
B#37WR56-11220−0.31WN5−0.41o−0.28WN5−0.26o>0WN5–6WN5o
B#56WR60-81510−0.01WN6−0.38o−0.27WN5−0.20o>0WN5–6WN6o
WR62a1670−0.09WN6−0.46o−0.20o/(h)>0WN5–6WN5oS99WN6o
B#85WR64-21480−0.03WN6−0.41o−0.32WN5−0.33o>0WN5–6WN6o
B#87WR64-31340+0.02WN6−0.22o/(h)−0.32WN5−0.19o>0WN5–6WN6o
B#88WR64-41930+0.13WN6−0.28o−0.26WN5−0.36o≫0WN6WN6o+OB
B#91WR64-51680+0.16WN6−0.29o−0.10WN6−0.25o≫0WN6WN6o
B#93WR64-62130+0.15WN6b−0.33o−0.16WN6b−0.38o>0WN6bWN6b
WR68a1680−0.11WN6−0.37o−0.13o/(h)>0WN5–6WN6oS99WN6o
B#107WR70-142760–0.16WN4–6b−0.43o−0.35WN6b−0.34o≃0WN4bWN4b
B#123WR70-151450−0.45WN4–5−0.50o−1.08WN2–4−0.55o>0WN5–6WN5o
B#132WR72-51370+0.02WN6−0.38o−0.26WN5:−0.26o≫0WN6WN6o
A#11WR75-311250+0.60:WN7–8−0.17o+0.39WN7–8−0.01o0.00aWN7WN7o
A#13WR75-30(1880)+0.25WN7−0.03o0.02aWN7WN6K15WN7o
B#154WR76-11(1260)+0.42WN7–8−0.08o0.05aWN7WN7o
WR93a1800−0.06WN6+0.27(h)+0.29h≫0WN6WN6M13WN6h
IDWR1.74 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(C iii 1.20/(He i-ii 1.70/(C iii 2.11/(C ii 0.99/SpTSpT
km s−1He ii 1.01)C iv 1.19)C iv 1.74)C iv 2.07)C iii 0.97)
E#3WR46-183100+0.14WC6–7−0.45WC7−0.71WC6–7−0.66WC4–7−1.62WC4–6WC6–7
B#51WR60-71800+0.28WC7–8−0.36WC8−0.70WC6–7−0.55WC7–8−1.36WC7–8WC7–8
B#105WR70-131300+0.62WC8–9+0.07WC8–9−0.36WC8−0.28WC8−1.21WC8–9WC8d
WR75aa1400+0.85WC9+0.23WC9−0.19WC8–9−0.07WC9−1.05WC9WC9dH05WC9
WR75c1350+1.33WC9+0.52WC9+0.23WC9+0.19WC9−0.88WC9WC9H05WC9
WR107a(2400)+0.01WC5−0.64WC5–7−0.69WC5–7−1.39WC5–8WC6S99WC5–7
IDWR1.01 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(P β/(He i 1.70/(Br γ/(He i+N iii 2.11/SpTSpT
km s−1He ii 1.01)He ii 1.16)He ii 1.69)He ii 2.19)N v 2.10)
B#13WR47-51000+0.08WN6−0.17(h)−0.55WN4−0.01(h)>0WN5–6WN6(h)
B#37WR56-11220−0.31WN5−0.41o−0.28WN5−0.26o>0WN5–6WN5o
B#56WR60-81510−0.01WN6−0.38o−0.27WN5−0.20o>0WN5–6WN6o
WR62a1670−0.09WN6−0.46o−0.20o/(h)>0WN5–6WN5oS99WN6o
B#85WR64-21480−0.03WN6−0.41o−0.32WN5−0.33o>0WN5–6WN6o
B#87WR64-31340+0.02WN6−0.22o/(h)−0.32WN5−0.19o>0WN5–6WN6o
B#88WR64-41930+0.13WN6−0.28o−0.26WN5−0.36o≫0WN6WN6o+OB
B#91WR64-51680+0.16WN6−0.29o−0.10WN6−0.25o≫0WN6WN6o
B#93WR64-62130+0.15WN6b−0.33o−0.16WN6b−0.38o>0WN6bWN6b
WR68a1680−0.11WN6−0.37o−0.13o/(h)>0WN5–6WN6oS99WN6o
B#107WR70-142760–0.16WN4–6b−0.43o−0.35WN6b−0.34o≃0WN4bWN4b
B#123WR70-151450−0.45WN4–5−0.50o−1.08WN2–4−0.55o>0WN5–6WN5o
B#132WR72-51370+0.02WN6−0.38o−0.26WN5:−0.26o≫0WN6WN6o
A#11WR75-311250+0.60:WN7–8−0.17o+0.39WN7–8−0.01o0.00aWN7WN7o
A#13WR75-30(1880)+0.25WN7−0.03o0.02aWN7WN6K15WN7o
B#154WR76-11(1260)+0.42WN7–8−0.08o0.05aWN7WN7o
WR93a1800−0.06WN6+0.27(h)+0.29h≫0WN6WN6M13WN6h
IDWR1.74 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(C iii 1.20/(He i-ii 1.70/(C iii 2.11/(C ii 0.99/SpTSpT
km s−1He ii 1.01)C iv 1.19)C iv 1.74)C iv 2.07)C iii 0.97)
E#3WR46-183100+0.14WC6–7−0.45WC7−0.71WC6–7−0.66WC4–7−1.62WC4–6WC6–7
B#51WR60-71800+0.28WC7–8−0.36WC8−0.70WC6–7−0.55WC7–8−1.36WC7–8WC7–8
B#105WR70-131300+0.62WC8–9+0.07WC8–9−0.36WC8−0.28WC8−1.21WC8–9WC8d
WR75aa1400+0.85WC9+0.23WC9−0.19WC8–9−0.07WC9−1.05WC9WC9dH05WC9
WR75c1350+1.33WC9+0.52WC9+0.23WC9+0.19WC9−0.88WC9WC9H05WC9
WR107a(2400)+0.01WC5−0.64WC5–7−0.69WC5–7−1.39WC5–8WC6S99WC5–7

Note. S99 (Shara et al. 1999), H05 (Hopewell et al. 2005), M13 (Miszalski et al. 2013), K15 (Kanarek et al. 2015).

alog Wλ (He i 2.112 + N iii 2.116/He ii 2.189).

Table 6.

Ratios of near-IR diagnostic lines for newly identified WR stars from NTT/SOFI spectroscopy plus revised near-IR classifications for previously known stars. Line strengths/widths are provided for He ii 1.012 μm (2.189 μm in parenthesis) or C iv 1.736 μm (1.190 μm in parenthesis) for WN and WC stars, respectively.

IDWR1.01 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(P β/(He i 1.70/(Br γ/(He i+N iii 2.11/SpTSpT
km s−1He ii 1.01)He ii 1.16)He ii 1.69)He ii 2.19)N v 2.10)
B#13WR47-51000+0.08WN6−0.17(h)−0.55WN4−0.01(h)>0WN5–6WN6(h)
B#37WR56-11220−0.31WN5−0.41o−0.28WN5−0.26o>0WN5–6WN5o
B#56WR60-81510−0.01WN6−0.38o−0.27WN5−0.20o>0WN5–6WN6o
WR62a1670−0.09WN6−0.46o−0.20o/(h)>0WN5–6WN5oS99WN6o
B#85WR64-21480−0.03WN6−0.41o−0.32WN5−0.33o>0WN5–6WN6o
B#87WR64-31340+0.02WN6−0.22o/(h)−0.32WN5−0.19o>0WN5–6WN6o
B#88WR64-41930+0.13WN6−0.28o−0.26WN5−0.36o≫0WN6WN6o+OB
B#91WR64-51680+0.16WN6−0.29o−0.10WN6−0.25o≫0WN6WN6o
B#93WR64-62130+0.15WN6b−0.33o−0.16WN6b−0.38o>0WN6bWN6b
WR68a1680−0.11WN6−0.37o−0.13o/(h)>0WN5–6WN6oS99WN6o
B#107WR70-142760–0.16WN4–6b−0.43o−0.35WN6b−0.34o≃0WN4bWN4b
B#123WR70-151450−0.45WN4–5−0.50o−1.08WN2–4−0.55o>0WN5–6WN5o
B#132WR72-51370+0.02WN6−0.38o−0.26WN5:−0.26o≫0WN6WN6o
A#11WR75-311250+0.60:WN7–8−0.17o+0.39WN7–8−0.01o0.00aWN7WN7o
A#13WR75-30(1880)+0.25WN7−0.03o0.02aWN7WN6K15WN7o
B#154WR76-11(1260)+0.42WN7–8−0.08o0.05aWN7WN7o
WR93a1800−0.06WN6+0.27(h)+0.29h≫0WN6WN6M13WN6h
IDWR1.74 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(C iii 1.20/(He i-ii 1.70/(C iii 2.11/(C ii 0.99/SpTSpT
km s−1He ii 1.01)C iv 1.19)C iv 1.74)C iv 2.07)C iii 0.97)
E#3WR46-183100+0.14WC6–7−0.45WC7−0.71WC6–7−0.66WC4–7−1.62WC4–6WC6–7
B#51WR60-71800+0.28WC7–8−0.36WC8−0.70WC6–7−0.55WC7–8−1.36WC7–8WC7–8
B#105WR70-131300+0.62WC8–9+0.07WC8–9−0.36WC8−0.28WC8−1.21WC8–9WC8d
WR75aa1400+0.85WC9+0.23WC9−0.19WC8–9−0.07WC9−1.05WC9WC9dH05WC9
WR75c1350+1.33WC9+0.52WC9+0.23WC9+0.19WC9−0.88WC9WC9H05WC9
WR107a(2400)+0.01WC5−0.64WC5–7−0.69WC5–7−1.39WC5–8WC6S99WC5–7
IDWR1.01 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(P β/(He i 1.70/(Br γ/(He i+N iii 2.11/SpTSpT
km s−1He ii 1.01)He ii 1.16)He ii 1.69)He ii 2.19)N v 2.10)
B#13WR47-51000+0.08WN6−0.17(h)−0.55WN4−0.01(h)>0WN5–6WN6(h)
B#37WR56-11220−0.31WN5−0.41o−0.28WN5−0.26o>0WN5–6WN5o
B#56WR60-81510−0.01WN6−0.38o−0.27WN5−0.20o>0WN5–6WN6o
WR62a1670−0.09WN6−0.46o−0.20o/(h)>0WN5–6WN5oS99WN6o
B#85WR64-21480−0.03WN6−0.41o−0.32WN5−0.33o>0WN5–6WN6o
B#87WR64-31340+0.02WN6−0.22o/(h)−0.32WN5−0.19o>0WN5–6WN6o
B#88WR64-41930+0.13WN6−0.28o−0.26WN5−0.36o≫0WN6WN6o+OB
B#91WR64-51680+0.16WN6−0.29o−0.10WN6−0.25o≫0WN6WN6o
B#93WR64-62130+0.15WN6b−0.33o−0.16WN6b−0.38o>0WN6bWN6b
WR68a1680−0.11WN6−0.37o−0.13o/(h)>0WN5–6WN6oS99WN6o
B#107WR70-142760–0.16WN4–6b−0.43o−0.35WN6b−0.34o≃0WN4bWN4b
B#123WR70-151450−0.45WN4–5−0.50o−1.08WN2–4−0.55o>0WN5–6WN5o
B#132WR72-51370+0.02WN6−0.38o−0.26WN5:−0.26o≫0WN6WN6o
A#11WR75-311250+0.60:WN7–8−0.17o+0.39WN7–8−0.01o0.00aWN7WN7o
A#13WR75-30(1880)+0.25WN7−0.03o0.02aWN7WN6K15WN7o
B#154WR76-11(1260)+0.42WN7–8−0.08o0.05aWN7WN7o
WR93a1800−0.06WN6+0.27(h)+0.29h≫0WN6WN6M13WN6h
IDWR1.74 μmlog Wλlog Wλlog Wλlog Wλlog WλOldRefNew
FWHM(He i 1.08/(C iii 1.20/(He i-ii 1.70/(C iii 2.11/(C ii 0.99/SpTSpT
km s−1He ii 1.01)C iv 1.19)C iv 1.74)C iv 2.07)C iii 0.97)
E#3WR46-183100+0.14WC6–7−0.45WC7−0.71WC6–7−0.66WC4–7−1.62WC4–6WC6–7
B#51WR60-71800+0.28WC7–8−0.36WC8−0.70WC6–7−0.55WC7–8−1.36WC7–8WC7–8
B#105WR70-131300+0.62WC8–9+0.07WC8–9−0.36WC8−0.28WC8−1.21WC8–9WC8d
WR75aa1400+0.85WC9+0.23WC9−0.19WC8–9−0.07WC9−1.05WC9WC9dH05WC9
WR75c1350+1.33WC9+0.52WC9+0.23WC9+0.19WC9−0.88WC9WC9H05WC9
WR107a(2400)+0.01WC5−0.64WC5–7−0.69WC5–7−1.39WC5–8WC6S99WC5–7

Note. S99 (Shara et al. 1999), H05 (Hopewell et al. 2005), M13 (Miszalski et al. 2013), K15 (Kanarek et al. 2015).

alog Wλ (He i 2.112 + N iii 2.116/He ii 2.189).

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