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Individual sheet: PACWB J104357–593252
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Spectral type(s): O2If* + O3.5V
Multiplicity:
Confirmed binary system
Period(s): undetermined
Orbital solution: no
Ref: Nelan et al. (2004), Maiz-Appelaniz et al. (2017)
Quality flag (Q): I
Comments:
This is one system among a few whose synchrotron emission region has been resolved using VLBI facilities (Benaglia et al. 2010, 2015).
Predictions on the high energy emission, from X-rays to gamma-rays, have been presented by del Palacio et al. (2016).
The analysis of Chandra and NuStar data obtained close to periastron passage has been presented by del Palacio et al (2020).
The analysis of its radio emission across periastron passage has be published by Benaglia et al. (2025).