Outbursts and Disk Variability in Be Stars (2018)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- DOI: 10.3847/1538-3881/aa9c7e
- Subjects: ESTRELAS; FOTOMETRIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v. 155, n. 2, p. 53, 2018
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
LABADIE-BARTZ, Jonathan e FERNANDES, Marcelo Borges e CARCIOFI, Alex Cavaliéri. Outbursts and Disk Variability in Be Stars. Astronomical Journal, v. 155, n. 2, p. 53, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-3881/aa9c7e. Acesso em: 23 jan. 2026. -
APA
Labadie-Bartz, J., Fernandes, M. B., & Carciofi, A. C. (2018). Outbursts and Disk Variability in Be Stars. Astronomical Journal, 155( 2), 53. doi:10.3847/1538-3881/aa9c7e -
NLM
Labadie-Bartz J, Fernandes MB, Carciofi AC. Outbursts and Disk Variability in Be Stars [Internet]. Astronomical Journal. 2018 ; 155( 2): 53.[citado 2026 jan. 23 ] Available from: https://doi.org/10.3847/1538-3881/aa9c7e -
Vancouver
Labadie-Bartz J, Fernandes MB, Carciofi AC. Outbursts and Disk Variability in Be Stars [Internet]. Astronomical Journal. 2018 ; 155( 2): 53.[citado 2026 jan. 23 ] Available from: https://doi.org/10.3847/1538-3881/aa9c7e - 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: 10.3847/1538-3881/aa9c7e (Fonte: oaDOI API)
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