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Infrared photometry of the probable triple WC4(+O?)+O8I: Wolf-Rayet system HD36402 (= BAT99-38) in the Large Magellanic Cloud (LMC) shows emissioncharacteristic of heated dust. The dust emission is variable on a time-scale ofyears, with a period near 4.7 yr, possibly associated with orbital motion ofthe O8 supergiant and the inner P ~ 3.03-d WC4+O binary. The phase of maximumdust emission is close to that of the X-ray minimum, consistent with bothprocesses being tied to colliding wind effects in an elliptical binary orbit.It is evident that Wolf-Rayet dust formation occurs also in metal-poorenvironments.

Variable dust formation by the colliding-wind Wolf-Rayet system HD 36402 in the Large Magellanic Cloud