AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks? (2014)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ESTRELAS; INTERFEROMETRIA
- Language: Inglês
- Imprenta:
- Publisher place: San Francisco
- Date published: 2014
- Source:
- Título: ASP Conference Series
- Volume/Número/Paginação/Ano: v. 487, p. 377-382, 2014
- Conference titles: Conference on Resolving the Future of Astronomy with Long-Baseline Interferometry
-
ABNT
ŠTEFL, S. et al. AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks?. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 03 jan. 2026. , 2014 -
APA
Štefl, S., Rivinius, T., Baade, D., & Carciofi, A. C. (2014). AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks? ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. -
NLM
Štefl S, Rivinius T, Baade D, Carciofi AC. AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks? ASP Conference Series. 2014 ; 487 377-382.[citado 2026 jan. 03 ] -
Vancouver
Štefl S, Rivinius T, Baade D, Carciofi AC. AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks? ASP Conference Series. 2014 ; 487 377-382.[citado 2026 jan. 03 ] - The 2008+ outburst of the Be star 28 CMA
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- Polarimetric observations of 'sigma' Orionis E
- Grid of supergiant B[e] models from HDUST radiative transfer
- Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data
- Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429
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