Search results for " stars: individual: V4046 Sgr"

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The Close T Tauri Binary System V4046 Sgr: Rotationally Modulated X-Ray Emission from Accretion Shocks

2012

We report initial results from a quasi-simultaneous X-ray/optical observing campaign targeting V4046 Sgr, a close, synchronous-rotating classical T Tauri star (CTTS) binary in which both components are actively accreting. V4046 Sgr is a strong X-ray source, with the X-rays mainly arising from high-density (n_e ~ 10^(11-12) cm^(-3)) plasma at temperatures of 3-4 MK. Our multiwavelength campaign aims to simultaneously constrain the properties of this X-ray emitting plasma, the large scale magnetic field, and the accretion geometry. In this paper, we present key results obtained via time-resolved X-ray grating spectra, gathered in a 360 ks XMM-Newton observation that covered 2.2 system rotatio…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral lineSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBinary starAstrophysics::Solar and Stellar AstrophysicsEmission spectrumBinary system010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics[PHYS]Physics [physics]accretion accretion disks stars: individual: V4046 Sgr stars: magnetic field stars: pre-main sequence stars: variables: T Tauri Herbig Ae/Be X-rays: stars010308 nuclear & particles physicsAstronomy and AstrophysicsPlasmaAccretion (astrophysics)StarsT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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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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