We present preliminary results of our X‐shooter survey in star forming regions. In this contribution we focus on subsamples of young stellar and sub‐stellar objects (YSOs) in the Lupus star forming region and in the TW Hya association. We show that the X‐shooter spectra are suitable for conducting several parallel studies such as YSO + disk fundamental parameters, accretion and outflow activity in the very low‐mass (VLM) and sub‐stellar regimes, as well as magnetic activity in young VLM YSOs, and Li abundance determinations. The capabilities of X‐shooter in terms of wide spectral coverage, resolution and limiting magnitudes, allow us to assess simultaneously the accretion/outflow, magnetic activity, and disk diagnostics, from the UV and opt...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
This work was co-funded under the Marie Curie Actions of the European Commission (FP7KCOFUND). A.S. ...
We present preliminary results of our X-shooter survey in star forming regions. In this contribution...
We present preliminary results of our X-shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
The mass accretion rate, Ṁacc, is a key quantity for the understanding of the physical processes gov...
The mass accretion rate, Ṁacc, is a key quantity for the understanding of the physical processes gov...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Star formation in the solar neighborhood is mainly traced by young stars in open clusters, ...
We present VLT/X-shooter observations of a sample of 36 accreting low-mass stellar and substellar ob...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
This work was co-funded under the Marie Curie Actions of the European Commission (FP7KCOFUND). A.S. ...
We present preliminary results of our X-shooter survey in star forming regions. In this contribution...
We present preliminary results of our X-shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
We present preliminary results of our X‐shooter survey in star forming regions. In this contribution...
The mass accretion rate, Ṁacc, is a key quantity for the understanding of the physical processes gov...
The mass accretion rate, Ṁacc, is a key quantity for the understanding of the physical processes gov...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Star formation in the solar neighborhood is mainly traced by young stars in open clusters, ...
We present VLT/X-shooter observations of a sample of 36 accreting low-mass stellar and substellar ob...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
This work was co-funded under the Marie Curie Actions of the European Commission (FP7KCOFUND). A.S. ...