activity
20172020
most citedPhysical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?

150 citations · 361 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.EP202031 cited

Constraining the radial drift of millimeter-sized grains in the protoplanetary disks in Lupus

L. Trapman, M. Ansdell, M. R. Hogerheijde +5

Recent ALMA surveys of protoplanetary disks have shown that for most disks the extent of the gas emission is greater than the extent of the thermal emission of the millimeter-sized…

astro-ph.SR201949 cited

Demographics of disks around young very low-mass stars and brown dwarfs in Lupus

E. Sanchis, L. Testi, A. Natta +15

We present new 890 continuum ALMA observations of 5 brown dwarfs (BDs) with infrared excess in Lupus I and III -- which, in combination with 4 BDs previously observed, allowed…

astro-ph.SR201965 cited

Stringent limits on the magnetic field strength in the disc of TW Hya: ALMA observations of CN polarisation

W. H. T. Vlemmings, B. Lankhaar, P. Cazzoletti +8

Despite their importance in the star formation process, measurements of magnetic field strength in proto-planetary discs remain rare. While linear polarisation of dust and molecula…

astro-ph.SR201966 cited

Spatial segregation of dust grains in transition disks. SPHERE observations of 2MASS J16083070-3828268 and RXJ1852.3-3700

M. Villenave, M. Benisty, W. R. F. Dent +27

Context. The mechanisms governing the opening of cavities in transition disks are not fully understood. Several processes have been proposed but their occurrence rate is still unkn…

astro-ph.SR2018

The ALMA Lupus protoplanetary disk survey: evidence for compact gas disks and molecular rings from CN

S. E. van Terwisga, E. F. van Dishoeck, P. Cazzoletti +10

The cyanide radical CN is abundant in protoplanetary disks, with line fluxes often comparable to those of CO. It is known to be sensitive to UV irradiation of the upper disk…

astro-ph.EP2017150 cited

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…