Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429 (2009)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ESTRELAS; ESPECTROMETRIA; FOTOMETRIA
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrofhysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 700, p. 209-220, 2009
-
ABNT
MIROSHNICHENKO, A.S et al. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal, v. 700, p. 209-220, 2009Tradução . . Acesso em: 03 jan. 2026. -
APA
Miroshnichenko, A. S., Chentsov, E. L., Klochkova, V. G., & Carciofi, A. C. (2009). Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal, 700, 209-220. -
NLM
Miroshnichenko AS, Chentsov EL, Klochkova VG, Carciofi AC. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal. 2009 ; 700 209-220.[citado 2026 jan. 03 ] -
Vancouver
Miroshnichenko AS, Chentsov EL, Klochkova VG, Carciofi AC. Toward understanding the B[e] phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429. The Astrofhysical Journal. 2009 ; 700 209-220.[citado 2026 jan. 03 ] - The 2008+ outburst of the Be star 28 CMA
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- Os efeitos da rotação estelar sobre o disco de estrelas Be's
- Um estudo teórico da evolução temporal das características polarimétricas de estrelas Be por meio do diagrama BJV
- V/R variations in Be shell stars
- Observational effects of stellar rotation on Be stars' disks
- Polarimetric observations of 'sigma' Orionis E
- Grid of supergiant B[e] models from HDUST radiative transfer
- AMBER high-spectral resolution interferometry of Be stars: more than just stars and disks?
- Fast ray-tracing algorithm for circumstellar structures (FRACS): II. Disc parameters of the B[e] supergiant CPD-57º 2874 from VLTI/MIDI data
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