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PROBING WOLF-RAYET WINDS: CHANDRA/HETG X-RAY SPECTRA OF WR 6
Journal article   Peer reviewed

PROBING WOLF-RAYET WINDS: CHANDRA/HETG X-RAY SPECTRA OF WR 6

David P. Huenemoerder, K. G. Gayley, W. -R. Hamann, R. Ignace, J. S. Nichols, L. Oskinova, A. M. T. Pollock, N. S. Schulz and T. Shenar
The Astrophysical journal, Vol.815(1), p.29
12/10/2015
DOI: 10.1088/0004-637X/815/1/29

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Abstract

With a deep Chandra/HETGS exposure of WR 6, we have resolved emission lines whose profiles show that the X-rays originate from a uniformly expanding spherical wind of high X-ray-continuum optical depth. The presence of strong helium-like forbidden lines places the source of X-ray emission at tens to hundreds of stellar radii from the photosphere. Variability was present in X-rays and simultaneous optical photometry, but neither were correlated with the known period of the system or with each other. An enhanced abundance of sodium revealed nuclear-processed material, a quantity related to the evolutionary state of the star. The characterization of the extent and nature of the hot plasma in WR 6 will help to pave the way to a more fundamental theoretical understanding of the winds and evolution of massive stars.
Astronomy & Astrophysics Physical Sciences Science & Technology

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