V615 Ori: a TTauri star with a resolved X-ray outflow

M. ORELLANA

San Juan

Workshop; X-ray Astrophysics - an advanced school for Latin American astronomers; 2011

Cospar (COmmittee on SPAce Research)

This is an application of the specific software for the XMM-Newton data archive acquisition and reduction that we have learned along this COSPAR workshop. The satellites in similar conditions, i.e. Chandra and Suzaku, has not pointed to this source. In this contribution we briefly present the obtained spectra of the source split into two resolved components, a jet-like feature and the TTauri star V615 Ori itself which we find  to show some contribution of non-thermal emission from base of the putative jet. The conclusion is that a further study is mandatory given the small number of X-ray jets resolved in TTauri stars, who usually are point-like sources due to either their coronal activity or the impact of accretion columns.