B. Silva, R. Azevedo, J. F. Gameiro, D. F. M. Folha
Abstract
Using data from FLAMES-GIRAFFE/VLT in two different bands (optical and infrared) we derived for 60 stars at least one accretion tracer. The accretion tracers used were: CaII infrared triplet, HeI 5875, Na-D and optical veiling. All these stars are from a subsample of COUP; therefore their X-rays properties are well known. In this work we correlate the (COUP) X-ray properties of these classical T Tauri stars with their spectral accretion tracers, finding that there is a correlation between the X-ray hardness ratio and the optical veiling.
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium.
AIP Conference Proceedings
Volume 1126, Page 373
2009 May
