Search results for " stars: imaging"

showing 2 items of 2 documents

The close classical T Tauri binary V4046 Sgr: Complex magnetic fields & distributed mass accretion

2011

We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes within the close binary system V4046 Sgr, hosting two partly-convective classical T Tauri stars of masses ~0.9 Msun and age ~12 Myr. In this paper, we present time-resolved spectropolarimetric observations collected in 2009 September with ESPaDOnS at the Canada-France-Hawaii Telescope (CFHT) and covering a full span of 7d or ~2.5 orbital/rotational cycles of V4046 Sgr. Small circularly polarised Zeeman signatures are detected in the photospheric absorption lines but not in the accretion-powered emission lines of V4046 Sgr, thereby demonstrating that both system components host lar…

stars: formation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]stars: individual: V4046 SgrAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsstars: imagingtechniques: polarimetricSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar Astrophysicsstars: rotation[SDU]Sciences of the Universe [physics]stars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysicstechniques: polarimetric stars: formation stars: imaging stars: individual: V4046 Sgr stars: magnetic fields stars: rotationAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics
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Non-stationary dynamo and magnetospheric accretion processes of the classical T Tauri star V2129 Oph

2011

We report here the first results of a multiwavelength campaign focussing on magnetospheric accretion processes of the classical T Tauri star V2129 Oph. In this paper, we present spectropolarimetric observations collected in 2009 July with ESPaDOnS at the Canada-France-Hawaii Telescope and contemporaneous photometry secured with the SMARTS facility. Circularly polarized Zeeman signatures are clearly detected, both in photospheric absorption and accretion-powered emission lines, from time-series of which we reconstruct new maps of the magnetic field, photospheric brightness and accretion-powered emission at the surface of V2129 Oph using our newest tomographic imaging tool - to be compared wi…

techniques: polarimetric stars: formation stars: imaging stars: individual: V2129 Oph stars: magnetic field stars: rotationSettore FIS/05 - Astronomia E Astrofisica
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