Search results for "Stars and Star Formation"

showing 3 items of 3 documents

Multi-wavelength diagnostics of accretion in an X-ray selected sample of CTTSs

2010

High resolution X-ray spectroscopy has revealed soft X-rays from high density plasma in Classical T-Tauri stars (CTTSs), probably arising from the accretion shock region. However, the mass accretion rates derived from the X-ray observations are consistently lower than those derived from UV/optical/NIR studies. We aim to test the hypothesis that the high density soft X-ray emission is from accretion by analysing optical accretion tracers from an X-ray selected sample of CTTSs in a homogeneous manner. We analyse optical spectra of a sample of CTTSs and calculate the accretion rates based on measuring optical emission lines. These are then compared to the accretion rates derived from the X-ray…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaX-rayStellar atmosphereStars and Star FormationFOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAccretion (astrophysics)StarsSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Earth and Planetary AstrophysicsSpectroscopyOrder of magnitudeAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Modeling accretion shocks on CTTSs and their X-ray emission

2009

Recent high spectral resolution X-ray observations of some CTTSs show the presence of high density plasma (ne=10^{11}-10^{13} cm^{-3}) at temperature T=2-3 MK. This plasma is likely heated up by an accretion shock on the star surface. We investigate this issue by an accurate modelling of the impact of an accretion stream onto the stellar chromosphere. Specifically, we present a large set of 1D hydrodynamical simulations aimed at investigating the physical properties of the system as a function of the density, and the velocity of the accretion stream and of the abundances of the heavy elements. We also synthesize the plasma X-ray emission from the simulations results, in order to link the ob…

Settore FIS/05 - Astronomia E AstrofisicaStars and Star Formation
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Modeling the X-ray emission from jets observed with Chandra

2009

Stars and Star Formation
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