150 citations · 634 across the 9 of their papers we have counts for
9 papers
High gas/dust size ratio indicating efficient radial drift in the mm-faint CX Tau disk
S. Facchini, E. F. van Dishoeck, C. F. Manara +7
The large majority of protoplanetary disks have very compact (AU) continuum emission at mm wavelengths. However, high angular resolution observations that resolve the…
A dust and gas cavity in the disc around CQ Tau revealed by ALMA
M. Giulia Ubeira Gabellini, Anna Miotello, Stefano Facchini +23
The combination of high resolution and sensitivity offered by ALMA is revolutionizing our understanding of protoplanetary discs, as their bulk gas and dust distributions can be stu…
On the millimetre continuum flux-radius correlation of proto-planetary discs
Giovanni P. Rosotti, Richard A. Booth, Marco Tazzari +3
A correlation between proto-planetary disc radii and sub-mm fluxes has been recently reported. In this Letter we show that the correlation is a sensitive probe of grain growth proc…
The time evolution of dusty protoplanetary disc radii: observed and physical radii differ
Giovanni P. Rosotti, Marco Tazzari, Richard A. Booth +3
Proto-planetary disc surveys conducted with ALMA are measuring disc radii in multiple star forming regions. The disc radius is a fundamental quantity to diagnose whether discs unde…
An Inner Disk in the Large Gap of the Transition Disk SR 24S
Paola Pinilla, Myriam Benisty, Paolo Cazzoletti +3
We report new Atacama Large Millimeter/sub-millimeter Array (ALMA) Band 3 observations at 2.75 mm of the TD around SR 24S with an angular resolution of 0.11'' 0.09''…
Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
M. Tazzari, L. Testi, A. Natta +9
The formation of planets strongly depends on the total amount as well as on the spatial distribution of solids in protoplanetary disks. Thanks to the improvements in resolution and…