Table 3.

Average values of derived temperatures of observed WR stars using β1 models. The WN-star values are compiled from Hamann et al. (2006), Oskinova et al. (2013), and Sander et al. (2014), while the WC-star values originate from Leuenhagen & Hamann (1998), De Marco & Crowther (1998) and Sander et al. (2012).

Spectral class:234567891011
WNT* [kK]a141.193.5789.9865.0957.2453.2843.5237.6525.7522.39
T2/3 [kK]a104.783.254.147.744.842.637.436.720.419.1
WCT* [kK]116.782.378.071.959.844.332.8531.5
T2/3 [kK]73.063.162.061.252.239.030.4529.5
Spectral class:234567891011
WNT* [kK]a141.193.5789.9865.0957.2453.2843.5237.6525.7522.39
T2/3 [kK]a104.783.254.147.744.842.637.436.720.419.1
WCT* [kK]116.782.378.071.959.844.332.8531.5
T2/3 [kK]73.063.162.061.252.239.030.4529.5

aThe same temperatures apply for the WNh-star models.

Table 3.

Average values of derived temperatures of observed WR stars using β1 models. The WN-star values are compiled from Hamann et al. (2006), Oskinova et al. (2013), and Sander et al. (2014), while the WC-star values originate from Leuenhagen & Hamann (1998), De Marco & Crowther (1998) and Sander et al. (2012).

Spectral class:234567891011
WNT* [kK]a141.193.5789.9865.0957.2453.2843.5237.6525.7522.39
T2/3 [kK]a104.783.254.147.744.842.637.436.720.419.1
WCT* [kK]116.782.378.071.959.844.332.8531.5
T2/3 [kK]73.063.162.061.252.239.030.4529.5
Spectral class:234567891011
WNT* [kK]a141.193.5789.9865.0957.2453.2843.5237.6525.7522.39
T2/3 [kK]a104.783.254.147.744.842.637.436.720.419.1
WCT* [kK]116.782.378.071.959.844.332.8531.5
T2/3 [kK]73.063.162.061.252.239.030.4529.5

aThe same temperatures apply for the WNh-star models.

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