A COORDINATED X-RAY AND OPTICAL CAMPAIGN OF THE NEAREST MASSIVE ECLIPSING BINARY, δ ORIONIS Aa. IV. A MULTIWAVELENGTH, NON-LTE SPECTROSCOPIC ANALYSIS

Eclipsing systems of massive stars allow one to explore the properties of their components in great detail. We perform a multi-wavelength, non-LTE analysis of the three components of the massive multiple system δ Ori A, focusing on the fundamental stellar properties, stellar winds, and X-ray charact...

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Bibliographic Details
Main Authors: Shenar, T. (Author), Oskinova, Lidia M. (Author), Hamann, W.-R (Author), Corcoran, M. F. (Author), Moffat, A. F. J. (Author), Pablo, H. (Author), Richardson, N. D. (Author), Waldron, W. L. (Author), Nichols, Joy S. (Author), Todt, H. (Author), Hoffman, J. L. (Author), Pollock, A. M. T. (Author), Negueruela, I. (Author), Huenemoerder, David P. (Contributor), Maiz Apellaniz, J. (Author), Naze, Y. (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-11-24T20:29:36Z.
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