Growth and dissipation of Be star discs in misaligned binary systems (2022)
- Authors:
- USP affiliated authors: CARCIOFI, ALEX CAVALIERI - IAG ; JONES, CHARLES - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stab3024
- Subjects: ESTRELAS BINÁRIAS; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v.509, p. 931-944, 2022
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
SUFFAK, M W e JONES, C E e CARCIOFI, Alex Cavaliéri. Growth and dissipation of Be star discs in misaligned binary systems. Monthly Notices of the Royal Astronomical Society, v. 509, p. 931-944, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3024. Acesso em: 22 jan. 2026. -
APA
Suffak, M. W., Jones, C. E., & Carciofi, A. C. (2022). Growth and dissipation of Be star discs in misaligned binary systems. Monthly Notices of the Royal Astronomical Society, 509, 931-944. doi:10.1093/mnras/stab3024 -
NLM
Suffak MW, Jones CE, Carciofi AC. Growth and dissipation of Be star discs in misaligned binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ;509 931-944.[citado 2026 jan. 22 ] Available from: https://doi.org/10.1093/mnras/stab3024 -
Vancouver
Suffak MW, Jones CE, Carciofi AC. Growth and dissipation of Be star discs in misaligned binary systems [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ;509 931-944.[citado 2026 jan. 22 ] Available from: https://doi.org/10.1093/mnras/stab3024 - Short-term variablility and mass loss in Be stars: II. Physical taxonomy of photometric variability observed by the Kepler spacecraft
- Multitechnique testing of the viscous decretion disk model - I. The stable and tenuous disk of the late-type Be star β CMi: (Corrigendum)
- Polarimetric observations of "sigma" Orionis E
- Report on the ESO/IAG/USP Workshop Circumstellar Dynamics at High Resolution held at Foz do Iguaçu, Paraná State, Brazil, 27 February - 2 March 2012
- Dynamical evolution of viscous disks around Be stars: I. Photometry
- The viscous decretion disk model of the classical Be star β CMi revisited
- Modelling the periodical variations in multiband polarization and photometry for discs of binary Be stars
- Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars
- HDUST3 — A chemically realistic, 3-D, NLTE radiative transfer code
- Investigating the circumstellar disk of the Be shell star 48 librae
Informações sobre o DOI: 10.1093/mnras/stab3024 (Fonte: oaDOI API)
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