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Table 2.

Parameters of WR 127 from different papers.

Ref. Mean HJD SpT P, days KWR(N V), km s−1 KO, km s−1 MWRsin3(i), M MOsin3(i), M
H45 2 431 281 WN5+early B 9.550 160 ± 10 (a) ∼65 ∼5.8 ∼21
GB67 2 434 201 WN5, WN5-A 9.5594 ∼162.5
M81 2 444 090 WN4+O 9.555 178 ± 7 99 ± 3 ∼9 ∼20
Ch11 2 453 195 WN5o+O8.5V 9.555 177 ± 5 99 ± 4 7.5 ± 0.6 13.4 ± 1.0
D22 2 458 256 WN3b+O9.5V 9.555 163 ± 5
Our data 2 460 170 WN3b+O9.5V 9.55465 182.7 ± 2.0 125 ± 5 11.8 ± 1.4 17.2 ± 1.4

Ref. Type i, ° MWR, M MO, M ĖWR, 10−5M yr−1

St. -Louis et al. (1988) Pol. 55.7 ± 8.2 16 ± 5 35 ± 11 ∼0.8
Lamontagne et al. (1996) Phot. 55.3 ± 4.7 ∼17 ∼36 1.4 ± 0.4 (b)
Our data (2022–2024) Spec. 55.5 21.0 ± 2.5 30.8 ± 2.4 2.6 ± 0.5

Notes. The upper table contains the results of spectroscopic observations of WR 127 obtained in different years. The lower table contains the observational results from which estimates of orbital inclination i and/or mass loss ĖWR rate are derived.

(a)

Calculated by us from radial velocity curve for N V by Hiltner (1945).

(b)

Based on the optical eclipse depth.

References. (H45) Hiltner (1945; GB67) Ganesh & Bappu (1967; M81) Massey (1981; Ch11) de La Chevrotière et al. (2011; D22) Dsilva et al. (2022).

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