activity
20152017
most citedGas density drops inside dust cavities of transitional disks around young stars observed with ALMA

174 citations · 397 across the 4 of their papers we have counts for

collaborators

5 papers

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…

astro-ph.SR201770 cited

The Sizes and Depletions of the Dust and Gas Cavities in the Transitional Disk J160421.7-213028

Ruobing Dong, Nienke van der Marel, Jun Hashimoto +18

We report ALMA Cycle 2 observations of 230 GHz (1.3 mm) dust continuum emission, and CO, CO, and CO J = 2-1 line emission, from the Upper Scorpius transitional…

astro-ph.SR2016

Evidence for a correlation between mass accretion rates onto young stars and the mass of their protoplanetary disks

C. F. Manara, G. Rosotti, L. Testi +13

A relation between the mass accretion rate onto the central young star and the mass of the surrounding protoplanetary disk has long been theoretically predicted and observationally…

astro-ph.GA20153 cited

Quantifying the gas inside dust cavities in transitional disks: implications for young planets

E. F. van Dishoeck, N. van der Marel, S. Bruderer +1

ALMA observations of a small sample of transitional disks with large dust cavities observed in Cycle 0 and 1 are summarized. The gas and dust surface density structures are inferre…

astro-ph.EP2015174 cited

Gas density drops inside dust cavities of transitional disks around young stars observed with ALMA

Nienke van der Marel, Ewine van Dishoeck, Simon Bruderer +2

Transitional disks with large dust cavities are important laboratories to study planet formation and disk evolution. Cold gas may still be present inside these cavities, but the qu…