http://arxiv.org/abs/1809.07581
A tomographic method, aiming at probing velocity fields at depth in stellar atmospheres, is applied to the red supergiant star {\mu} Cep and to snapshots of 3D radiative-hydrodynamics simulation in order to constrain atmospheric motions and relate them to photometric variability.
K. Kravchenko, A. Chiavassa, S. Eck, et. al.
Fri, 21 Sep 18
20/63
Comments: 2 pages, 2 figures, accepted as Proceedings of IAU Symposium No. 343, 2018
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