Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars (2017)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Astronomical Society of the Pacific
- Publisher place: San Francisco
- Date published: 2017
- ISBN: 9781583819005
- Conference titles: International Conference on Studies of the B[e] Phenomenon
-
ABNT
BAADE, D et al. Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars. 2017, Anais.. San Francisco: Astronomical Society of the Pacific, 2017. Disponível em: http://www.aspbooks.org/a/volumes/table_of_contentes/508. Acesso em: 14 maio 2025. -
APA
Baade, D., Rivinius, T., Pigulski, A., Carciofi, A. C., & Best, A. (2017). Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars. In . San Francisco: Astronomical Society of the Pacific. Recuperado de http://www.aspbooks.org/a/volumes/table_of_contentes/508 -
NLM
Baade D, Rivinius T, Pigulski A, Carciofi AC, Best A. Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars [Internet]. 2017 ;[citado 2025 maio 14 ] Available from: http://www.aspbooks.org/a/volumes/table_of_contentes/508 -
Vancouver
Baade D, Rivinius T, Pigulski A, Carciofi AC, Best A. Difference frequencies of non-radial pulsation modes and repetitive outbursts in classical Be stars [Internet]. 2017 ;[citado 2025 maio 14 ] Available from: http://www.aspbooks.org/a/volumes/table_of_contentes/508 - Estudo sistemático dos locais de formação dos observáveis em discos de estrelas Be
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- A new diagnostic of the radial density structure of Be disks
- Grid of models for B[e] supergiants
- The viscous decretion disc properties of 80 Be stars
- Disk-loss and disk renewal phases in classical Be stars III: Modeling effects of disk structure
- Monitoramento da variabilidade polarimétrica de Delta Scorpii
- Viscous discks in Be stars
- The Be star Achernar and its circumstellar environement
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