http://arxiv.org/abs/1711.08394
In this contribution, we present BRITE observations of the early-B supergiants $\epsilon$ Ori and $\kappa$ Ori. We perform a preliminary analysis of the data acquired over the first two Orion observing runs. We evaluate whether they are compatible with co-rotating bright spots and discuss the challenges of such an approach.
A. David-Uraz, G. Wade, A. Moffat, et. al.
Thu, 23 Nov 17
10/52
Comments: 6 pages, 3 figures, to be published in the proceedings of the 3rd BRITE Science Conference held in Saint-Michel-des-Saints (QC, Canada), 2017 August 7-10 — Proceedings of the Polish Astronomical Society
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