6533b83afe1ef96bd12a75fd

RESEARCH PRODUCT

The Deep Rho Ophiuchi XMM-Newton Observation (DROXO)

S. SciortinoI. PillitteriF. DamianiEttore FlaccomioG. MicelaB. StelzerF. FavataG. GiardinoN. GrossoT. MontmerleF. PallaL. Testi

subject

[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]stars : individual : rho Ophiuchistars : formation[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]X-rays : star

description

International audience; We present the X-ray data and the analysis status of the DROXO (Deep Rho Oph XMM-Newton Observation) project, aimed to mainly characterize the spectro-variability properties of YSOs in the nearby and very young ρ Oph star forming region. We focus on a few selected initial scientific results for few interesting YSOs, such as Elias 29 and YLW16A. In Elias 29 we see the 6.4 keV fluorescent Fe line as already reported in literature, whereas in YLW16A we do not detect the fluorescent line at odd with previous findings. Hence we conclude that the line intensity does change with time (and/or physical conditions).

https://hal.archives-ouvertes.fr/hal-00104984