Seismological analysis of intermediate mass stars with moderate rotation (2012)
- Authors:
- Autor USP: PACHECO, EDUARDO JANOT - IAG
- Unidade: IAG
- Subjects: ESTRELAS; SISMOLOGIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Sociedade Astronômica Brasileira
- Publisher place: São Paulo
- Date published: 2012
- Conference titles: Reunião Anual da Sociedade Astronômica Brasileira
-
ABNT
RÍMULO, Leandro Rocha e PACHECO, Eduardo Janot e ANDRADE, Laerte Brandão Paes de. Seismological analysis of intermediate mass stars with moderate rotation. 2012, Anais.. São Paulo: Sociedade Astronômica Brasileira, 2012. . Acesso em: 10 jan. 2026. -
APA
Rímulo, L. R., Pacheco, E. J., & Andrade, L. B. P. de. (2012). Seismological analysis of intermediate mass stars with moderate rotation. In . São Paulo: Sociedade Astronômica Brasileira. -
NLM
Rímulo LR, Pacheco EJ, Andrade LBP de. Seismological analysis of intermediate mass stars with moderate rotation. 2012 ;[citado 2026 jan. 10 ] -
Vancouver
Rímulo LR, Pacheco EJ, Andrade LBP de. Seismological analysis of intermediate mass stars with moderate rotation. 2012 ;[citado 2026 jan. 10 ] - First dedicated observations of the isolated neutron star in the carina nebula
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- Automated supervised classification of variable stars in the CoRot programme: method and application to the first four exoplanet fields
- The BO.5IVe CoRot target HD49330: I. Photometric analysis from CoRoT data
- An study of v sin i distribution of Be stars
- Stellar parameters for a sample of Be stars
- Photometric and spectroscopic variability of the Be star HD 171219
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