Analysis of information sources in references of the Wikipedia article "GW Orionis" in English language version.
When we combined the RV constraints with the disk-based constraint on Mtot, we found stellar masses of MA = 2.7 M⊙, MB = 1.7 M⊙, and MC = 0.9 M⊙, to a precision of ± 0.3 M⊙
The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M⊙, respectively (Czekala et al. 2017)
When we combined the RV constraints with the disk-based constraint on Mtot, we found stellar masses of MA = 2.7 M⊙, MB = 1.7 M⊙, and MC = 0.9 M⊙, to a precision of ± 0.3 M⊙
The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M⊙, respectively (Czekala et al. 2017)
When we combined the RV constraints with the disk-based constraint on Mtot, we found stellar masses of MA = 2.7 M⊙, MB = 1.7 M⊙, and MC = 0.9 M⊙, to a precision of ± 0.3 M⊙
The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M⊙, respectively (Czekala et al. 2017)
When we combined the RV constraints with the disk-based constraint on Mtot, we found stellar masses of MA = 2.7 M⊙, MB = 1.7 M⊙, and MC = 0.9 M⊙, to a precision of ± 0.3 M⊙