Revealing the structure of the outer disks of Be stars

Context. The structure of the inner parts of Be star disks (≲ 20 stellar radii) is well explained by the viscous decretion disk (VDD) model, which is able to reproduce the observable properties of most of the objects studied so far. The outer parts, on the other hand, are not observationally well-ex...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2017-05, Vol.601, p.A74
Hauptverfasser:	Klement, R., Carciofi, A. C., Rivinius, T., Matthews, L. D., Vieira, R. G., Ignace, R., Bjorkman, J. E., Mota, B. C., Faes, D. M., Bratcher, A. D., Curé, M., Štefl, S.
Format:	Artikel
Sprache:	eng
Schlagworte:	binaries: general Binary stars circumstellar matter Computer simulation Mathematical models Model testing Radiative transfer Radio radio continuum: stars Spectra Spectral energy distribution Stars stars: emission-line submillimeter: stars Tidal energy Tidal power Wavelengths
Online-Zugang:	Volltext
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