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 do periódico: The Astrophysical Journal
- ISSN: 0004-637X
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
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: 28 jan. 2023. -
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 2023 jan. 28 ] 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 2023 jan. 28 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf - Outbursts and Disk Variability in Be Stars
- Orbital solution leading to an acceptable interpretation for the enigmatic gamma-ray binary HESS J0632+057
- Short-term variablility and mass loss in Be stars: II. Physical taxonomy of photometric variability observed by the Kepler spacecraft
- Variable rotational line broadening in the Be star Achernar
- Polarimetric observations of "sigma" Orionis E
- The photosphere and circumstellar environment of the Be star Achernar
- 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
- The 2008+ outburst of the Be star 28 CMa: a multi-instrument study
- Dynamical evolution of viscous disks around Be stars: I. Photometry
- Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe)
Informações sobre o DOI: 10.3847/0004-637X/826/1/81 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas