Search results for " stars: individual: TWA 5"

showing 1 items of 1 documents

XMM-Newton spectroscopy of the metal depleted T Tauri star TWA 5

2005

We present results of X-ray spectroscopy for TWA 5, a member of the young TW Hydrae association, observed with XMM-Newton. TWA~5 is a multiple system which shows Halpha emission, a signature typical of classical T Tauri stars, but no infrared excess. From the analysis of the RGS and EPIC spectra, we have derived the emission measure distribution vs. temperature of the X-ray emitting plasma, its abundances, and the electron density. The characteristic temperature and density of the plasma suggest a corona similar to that of weak-line T Tauri stars and active late-type main sequence stars. TWA 5 also shows a low iron abundance (~0.1 times the solar photospheric one) and a pattern of increasin…

PhysicsInfrared excessAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoronaSpectral lineAccretion (astrophysics)StarsT Tauri starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceTW HydraeX-rays: stars techniques: spectroscopic stars: activity stars: abundances stars: pre-main sequence stars: individual: TWA 5Main sequenceAstronomy & Astrophysics
researchProduct