6533b881fe1ef96bd12d8cd2

RESEARCH PRODUCT

XMM spectroscopy of TWA 5

C. ArgiroffiA. MaggioG. PeresB. StelzerR. Neuhaeuser

subject

Astrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray sourcesobservational astronomyPre main sequence starsX ray sourcesStellar AstronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPre-main sequence starsMultiple starsNatural SciencescosmologyAstrophysics::Galaxy AstrophysicsSpectroscopy

description

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 H{alpha} emission, a signature typical of classical T Tauri stars, but no infrared excess. From this 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.

10.26093/cds/vizier.34391149https://doi.org/http://doi.org/10.26093/cds/vizier.34391149