Rapidly accelerating clumps in the winds of the very hot WNE Stars

Details Rapidly accelerating clumps in the winds of the very hot WNE Stars Rapidly accelerating clumps in the winds of the very hot WNE Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cihw.conf..163c&link_type=abstract

Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Hamann, Wol

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Scientific paper

We study the time variability of emission lines in three WNE stars : WR 2 (WN2), WR 3 (WN3ha) and WR152 (WN3). While WR 2 shows no variability above the noise level, the other stars do show variation, which are like other WR stars in WR 152 but very fast in WR 3. From these motions, we deduce a value of β ˜1 for WR 3 that is like that seen in O stars and β ˜2 3 for WR 152, that is intermediate between other WR stars and WR 3.

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