# Be discs in coplanar circular binaries: Phase-locked variations of emission lines

## TL;DR

This paper models the structure and emission line variability of Be star decretion discs in coplanar circular binaries, revealing phase-locked V/R ratio variations caused by tidal interactions, aiding binary system identification.

## Contribution

It introduces a combined hydrodynamics and radiative transfer approach to simulate and analyze emission line variations in binary Be star discs, highlighting phase-locked V/R variability.

## Key findings

- Disc structure features two spiral arms.
- V/R ratio shows two maxima per orbital cycle.
- Phase-locked emission line variability can indicate binary presence.

## Abstract

The first results of radiative transfer calculations on decretion discs of binary Be stars are presented. A smoothed particle hydrodynamics code computes the structure of Be discs in coplanar circular binary systems for a range of orbital and disc parameters. The resulting disc configuration consists of two spiral arms, and can be given as input into a Monte Carlo code, which calculates the radiative transfer along the line of sight for various observational coordinates. Making use of the property of steady disc structure in coplanar circular binaries, observables are computed as functions of the orbital phase. Orbital-phase series of line profiles are given for selected parameter sets under various viewing angles, to allow comparison with observations. Flat-topped profiles with and without superimposed multiple structures are reproduced, showing, for example, that triple-peaked profiles do not have to be necessarily associated with warped discs and misaligned binaries. It is demonstrated that binary tidal effects give rise to phase-locked variability of the violet-to-red (V/R) ratio of hydrogen emission lines. The V/R ratio exhibits two maxima per cycle; in certain cases those maxima are equal, leading to a clear new V/R cycle every half orbital period. This study opens a way in identifying binaries and in constraining the parameters of binary systems that exhibit phase-locked variations induced by tidal interaction with a companion star.