Tomographic simulations of accretion disks in cataclysmic variables-flickering and wind (2008)
- Authors:
- Autor USP: DIAZ, MARCOS PEREZ - IAG
- Unidade: IAG
- Subjects: DISCOS DE ACRESÇÃO; ESTRELAS BINÁRIAS
- Language: Inglês
- Imprenta:
- Source:
- Título: Publications of the Astronomical Society of Japan
- Volume/Número/Paginação/Ano: v.60, p. 327-335, 2008
-
ABNT
RIBEIRO, Fabíola M. A e DIAZ, Marcos Perez. Tomographic simulations of accretion disks in cataclysmic variables-flickering and wind. Publications of the Astronomical Society of Japan, v. 60, p. 327-335, 2008Tradução . . Acesso em: 13 mar. 2026. -
APA
Ribeiro, F. M. A., & Diaz, M. P. (2008). Tomographic simulations of accretion disks in cataclysmic variables-flickering and wind. Publications of the Astronomical Society of Japan, 60, 327-335. -
NLM
Ribeiro FMA, Diaz MP. Tomographic simulations of accretion disks in cataclysmic variables-flickering and wind. Publications of the Astronomical Society of Japan. 2008 ;60 327-335.[citado 2026 mar. 13 ] -
Vancouver
Ribeiro FMA, Diaz MP. Tomographic simulations of accretion disks in cataclysmic variables-flickering and wind. Publications of the Astronomical Society of Japan. 2008 ;60 327-335.[citado 2026 mar. 13 ] - Detection of the secondary eclipse of Qatar-1b in the Ks band
- The radius inflation problem in short-period low-mass binaries: a large sample analysis
- Infrared spectroscopy of the supersoft X-ray source MR Vel
- Low-mass eclipsing binaries in the WFCAM transit survey
- Spectral synthesis of accretion disk winds in cataclysmic variables
- Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08° 3, HQ monocerotis and ST chamaeleontis
- Spectroscopy and photometry of the pre-cataclysmic binary PG 1026+002
- UV emission and spectral synthesis of accretion disks in non-magnetic cataclysmic variables
- HR Del remnant anatomy using 2D spectral data and 3D photoionization shell models
- Low-mass eclipsing binaries in the WFCAM Transit Survey: the persistence of the M-dwarf radius inflation problem
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
