SIMBAD references

2013MNRAS.431.1160W - Mon. Not. R. Astron. Soc., 431, 1160-1166 (2013/May-2)

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

WILLIAMS P.M., CHU Y.-H., GRUENDL R.A. and GUERRERO M.A.

Abstract (from CDS):

Infrared photometry of the probable triple WC4(+O{quest})+O8I: Wolf-Rayet system HD 36402 (= BAT99-38) in the Large Magellanic Cloud shows emission characteristic of heated dust. The dust emission is variable on a time-scale of years, with a period near 4.7 yr, possibly associated with orbital motion of the O8 supergiant and the inner P ≃ 3.03-d WC4+O binary. The phase of maximum dust emission is close to that of the X-ray minimum, consistent with both processes being tied to colliding wind effects in an elliptical binary orbit. It is evident that Wolf-Rayet dust formation occurs also in metal-poor environments.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): stars: individual: HD 36402 - stars: winds, outflows - stars: Wolf-Rayet - infrared: stars - X-rays: binaries

Status at CDS:  

CDS comments: IR1 (p.1161) is [CGC2005] YSO-2 in Simbad.

Simbad objects: 17

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2020.05.28-14:50:35

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