Growth and dissipation of Be star discs in misaligned binary systems Article Swipe
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· 2021
· Open Access
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· DOI: https://doi.org/10.1093/mnras/stab3024
We use a three-dimensional smoothed particle hydrodynamics code to simulate growth and dissipation of Be star discs in systems where the binary orbit is misaligned with respect to the spin axis of the primary star. We investigate six different scenarios of varying orbital period and misalignment angle, feeding the disc at a constant rate for 100 orbital periods, and then letting the disc dissipate for 100 orbital periods. During the disc growth phase, we find that the binary companion tilts the disc away from its initial plane at the equator of the primary star before settling to a constant orientation after 40–50 orbital periods. While the mass-injection into the disc is ongoing, the tilting of the disc can cause material to reaccrete on to the primary star prematurely. Once disc dissipation begins, usually the disc precesses about the binary companion’s orbital axis with precession periods ranging from 20 to 50 orbital periods. In special cases, we detect phenomena of disc tearing, as well as Kozai–Lidov oscillations of the disc. These oscillations reach a maximum eccentricity of about 0.6, and a minimum inclination of about 20○ with respect to the binary’s orbit. We also find the disc material to have highly eccentric orbits beyond the transition radius, where the disc changes from being dominated by viscous forces, to heavily controlled by the companion star, in contrast to its nearly circular motion inwards of the transition radius. Finally, we offer predictions to how these changes will affect Be star observables.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stab3024
- OA Status
- green
- Cited By
- 33
- References
- 61
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W3206910181
Raw OpenAlex JSON
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https://openalex.org/W3206910181Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stab3024Digital Object Identifier
- Title
-
Growth and dissipation of Be star discs in misaligned binary systemsWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2021Year of publication
- Publication date
-
2021-10-19Full publication date if available
- Authors
-
M. W. Suffak, C. E. Jones, A. C. CarciofiList of authors in order
- Landing page
-
https://doi.org/10.1093/mnras/stab3024Publisher landing page
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
-
https://arxiv.org/pdf/2110.08344Direct OA link when available
- Concepts
-
Physics, Orbital plane, Precession, Orbit (dynamics), Astrophysics, Orbital eccentricity, RADIUS, Binary star, Circular orbit, Accretion (finance), Orbital decay, Circumbinary planet, Eccentricity (behavior), Orbital inclination, Astronomy, Binary number, Stars, Computer science, Mathematics, Political science, Arithmetic, Aerospace engineering, Satellite, Computer security, Law, EngineeringTop concepts (fields/topics) attached by OpenAlex
- Cited by
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33Total citation count in OpenAlex
- Citations by year (recent)
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2025: 8, 2024: 7, 2023: 10, 2022: 5, 2021: 3Per-year citation counts (last 5 years)
- References (count)
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61Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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| publication_date | 2021-10-19 |
| publication_year | 2021 |
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