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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Be discs in binary systems - I. Coplanar orbits

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Author(s):
Panoglou, Despina ; Carciofi, Alex C. ; Vieira, Rodrigo G. ; Cyr, Isabelle H. ; Jones, Carol E. ; Okazaki, Atsuo T. ; Rivinius, Thomas
Total Authors: 7
Document type: Journal article
Source: Monthly Notices of the Royal Astronomical Society; v. 461, n. 3, p. 2616-2629, SEP 21 2016.
Web of Science Citations: 19
Abstract

Be stars are surrounded by outflowing circumstellar matter structured in the form of decretion discs. They are often members of binary systems, where it is expected that the decretion disc interacts both radiatively and gravitationally with the companion. In this work we study how various orbital (period, mass ratio and eccentricity) and disc (viscosity) parameters affect the disc structure in coplanar binaries. The main effects of the secondary on the disc are its truncation and the accumulation of material inwards of truncation. We find two limiting cases with respect to the effects of eccentricity: in circular or nearly circular prograde orbits, the disc maintains a rotating, constant in shape, configuration, which is locked to the orbital phase. The disc structure appears smaller in size, more elongated and more massive for small viscosity parameter, small orbital separation and/or high mass ratio. In highly eccentric orbits, the effects are more complex, with the disc structure strongly dependent on the orbital phase. We also studied the effects of binarity in the disc continuum emission. Since the infrared and radio SED are sensitive to the disc size and density slope, the truncation and matter accumulation result in considerable modifications in the emergent spectrum. We conclude that binarity can serve as an explanation for the variability exhibited in observations of Be stars, and that our model can be used to detect invisible companions. (AU)

FAPESP's process: 13/16801-2 - Modelling the formation and evolution of inflowing and outflowing gaseous disks around stars
Grantee:Despina Panoglou
Support Opportunities: Scholarships in Brazil - Post-Doctoral
FAPESP's process: 15/17967-7 - Viscous decretion disks: theory and observations
Grantee:Alex Cavaliéri Carciofi
Support Opportunities: Regular Research Grants
FAPESP's process: 09/54006-4 - A computer cluster for the Astronomy Department of the University of São Paulo Institute of Astronomy, Geophysics and Atmospheric Sciences and for the Cruzeiro do Sul University Astrophysics Center
Grantee:Elisabete Maria de Gouveia Dal Pino
Support Opportunities: Multi-user Equipment Program
FAPESP's process: 12/20364-4 - Beyond dust survival: the inner regions of protoplanetary disks
Grantee:Rodrigo Georgetti Vieira
Support Opportunities: Scholarships in Brazil - Post-Doctoral