Investigating the circumstellar disk of the Be shell star 48 librae (2016)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- DOI: 10.3847/0004-637X/826/1/81
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
SILAJ, j e JONES, C. E e CARCIOFI, Alex Cavaliéri. Investigating the circumstellar disk of the Be shell star 48 librae. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf. Acesso em: 22 jan. 2026. -
APA
Silaj, j, Jones, C. E., & Carciofi, A. C. (2016). Investigating the circumstellar disk of the Be shell star 48 librae. The Astrophysical Journal. doi:10.3847/0004-637X/826/1/81 -
NLM
Silaj j, Jones CE, Carciofi AC. Investigating the circumstellar disk of the Be shell star 48 librae [Internet]. The Astrophysical Journal. 2016 ;[citado 2026 jan. 22 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf -
Vancouver
Silaj j, Jones CE, Carciofi AC. Investigating the circumstellar disk of the Be shell star 48 librae [Internet]. The Astrophysical Journal. 2016 ;[citado 2026 jan. 22 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf - 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
- O fenômeno de inversão de fases interferométricas em estrelas Be
Informações sobre o DOI: 10.3847/0004-637X/826/1/81 (Fonte: oaDOI API)
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