We present preliminary results of our X-shooter survey in star forming regions. In this contribution we focus on sub-samples 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 op...
Context. Measurements of the fraction of disk-bearing stars in clusters as a function of age indicat...
We present high-quality, medium-resolution X-shooter/VLT spectra in the range 300−2500 nm for a samp...
We discuss accretion and outflow properties of three very low-mass young stellar objects based on br...
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...
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...
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...
We present high-quality, medium-resolution X-shooter/VLT spectra in the range 300−2500 nm for a samp...
We discuss accretion and outflow properties of three very low-mass young stellar objects based on br...
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...
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...
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...
We present high-quality, medium-resolution X-shooter/VLT spectra in the range 300−2500 nm for a samp...
We discuss accretion and outflow properties of three very low-mass young stellar objects based on br...