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Table 5.

Parameters of HD 77581 derived by different authors.

Reference log L EB − V T vrot sin i log g
[L] [mag] [kK] [km s−1] [cgs] Comments
Wickramasinghe et al. (1974) 0.75 20–28 ∼90 2.5–3.0 RV, spectrum and reddening
Mikkelsen & Wallerstein (1974) (MW74) 5.2 0.75 22 130 2.64–2.80
Lamers et al. (1976) 26.3
Ammann & Mauder (1978) 89 ± 5 HeI line fitting
Conti (1978) (C78) 5.7 0.73 26 (MW74)
Dupree et al. (1980) (C78) 0.7 (C78)
Sadakane et al. (1985) 5.53 25 ± 1
Vanbeveren et al. (1993) 5.5–5.7 26 130 2.75–2.76
Zuiderwijk (1995) 116 ± 6 HeI line profiles
Howarth et al. (1997) 114 Cross-correlating IUE spectra
Fraser et al. (2010) (F10) 26.5 56 2.90 Arrive at mass of 40 M
Falanga et al. (2015) 130.3 ± 0.2 From system geometry
Krtička et al. (2015) 5.63 27
Giménez-García et al. (2016) 5.5 ± 0.1 0.77 ± 0.05 24.4 ± 1.0 (F10) 2.86 ± 0.10 Uses d = 2.0 ± 0.2 kpc
Sander et al. (2018), no X-rays 5.485 23.5 (F10) 2.84 same distance as above
– ditto –, moderate X-ray illum. – ditto – 23.5 – ditto –
– ditto –, strong X-ray illum. – ditto – 23.8 – ditto –
This work (Sect. 5.5) 5.8–6.2 0.689 ± 0.018 33.7 ± 5.2 3.28 ± 0.19 Uses d = 1.99 kpc

Notes. See Sect. 3.2.3 for notes on the different approaches used. For Giménez-García et al. (2016) and Sander et al. (2018), the temperature we report here as T corresponds to the parameter T2/3 as defined in the PoWR code used by these publications. For mass and radius estimates, see Table 4.

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