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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.)

Modelling the periodical variations in multiband polarization and photometry for discs of binary Be stars

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Panoglou, Despina [1] ; Fernandes, Marcelo Borges [1] ; Baade, Dietrich [2] ; Faes, Daniel M. [3] ; Rivinius, Thomas [4] ; Carciofi, Alex C. [3] ; Okazaki, Atsuo T. [5]
Total Authors: 7
[1] Observ Nacl, Rua Gen Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ - Brazil
[2] European Org Astron Res Southern Hemisphere, Karl Schwarzschild Str 2, D-85748 Garching - Germany
[3] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226, BR-05508900 Sao Paulo, SP - Brazil
[4] European Org Astron Res Southern Hemisphere, Santiago 19001 - Chile
[5] Hokkai Gakunen Univ, Fac Engn, Sapporo, Hokkaido 0628605 - Japan
Total Affiliations: 5
Document type: Journal article
Source: Monthly Notices of the Royal Astronomical Society; v. 486, n. 4, p. 5139-5157, JUL 2019.
Web of Science Citations: 1

The tidal interaction of a Be star with a binary companion forms two spiral arms that cause orbital modulation of the Be disc structure. The aim of this work is to identify observables in which this modulation is apparent. The structure of a Be disc in a coplanar circular binary system is computed with a smoothed-particle hydrodynamics code, and a radiation transfer code calculates the spectral energy distribution. Line depolarization was confirmed, with polarization profiles nearly reverse to emission-line profiles. The continuum flux maximizes for pole-on discs, but photometric variability maximizes for edge-on discs. The linear polarization exhibits one or two maxima per orbital cycle. While polarization variability in visible passbands is important only al low inclinations, infrared bands may demonstrate high orbital variability even at large inclinations. More evident is the modulation in the polarization angle (PA) for low: inclinations. The latter can be used to track azimuthal asymmetries for pole-on discs, where the spectroscopic variability in the violet-to-red (V/R) emission-component ratio disappears. PA reversals coincide with phases where V/R = 1, tracking lines of sight directed towards regions where the approaching and receding arms overlap. Continuum flux and polarization are mostly in phase for neighbouring wavelength regions. It is suggested that studies of non-symmetric discs distorted by tidal forces from a secondary star may be used to study disc variabilities of other origins. (AU)

FAPESP's process: 16/16844-1 - Systems Engineering for GMACS: GMT AT-13 Project
Grantee:Daniel Moser Faes
Support type: Scholarships in Brazil - Post-Doctorate
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 type: Multi-user Equipment Program