A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavelengths requires baselines up to similar to 15 km. To develop and test ...
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With its three spectrograph arms, X-shooter provides simultaneous wavelength coverage from ~300 to ~2480nm. For most of the targets, slits of 10/09/09 were used in the UVB/VIS/NIR arms, respectively, yielding resolving powers of 5100/8800/5600. Only ...
ALMA observations of DG Tau B were performed during Cycle 4 in August 2017 in an extended configuration with baselines ranging from 17m to 3.7km. The total integration time amounted to 88-minutes. The bandpass was calibrated with the quasar J0510+180...
All the data used in this paper were acquired with the X-shooter spectrograph at the VLT. The capabilities of X-shooter in terms of wide spectral coverage (310-2500nm), resolution and limiting magnitudes allow us to assess simultaneously the mass acc...
We used the ^12^CO (1-0) spectral cube to extract a catalogue of molecular clouds by using the SCIMES algorithm (Colombo et al., 2015MNRAS.454.2067C). A table of the physical properties of the molecular clouds are provided in the file table1.dat
The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of planet formation, these processes are best probed spectroscopically. ...
Observations of protoplanetary disks around very low-mass stars and brown dwarfs remain challenging and little is known about their properties. The disk around CIDA1 ($\sim$0.1-0.2$M_\odot$) is one of the very few known disks that host a large cavity...
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International audience