activity
20082018
most citedALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses

617 citations · 2.7k across the 22 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2018★ 10 cited

Exploring DCO as a tracer of thermal inversion in the disk around the Herbig Ae star HD163296

V. N. Salinas, M. R. Hogerheijde, N. M. Murillo +4

We aim to reproduce the DCO emission in the disk around HD163296 using a simple 2D chemical model for the formation of DCO through the cold deuteration channel and a parame…

astro-ph.SR2017★ 58 cited

DCO, DCN and ND reveal three different deuteration regimes in the disk around the Herbig Ae star HD163296

V. N. Salinas, M. R. Hogerheijde, G. S. Mathews +4

The formation pathways of deuterated species trace different regions of protoplanetary disks and may shed light into their physical structure. We aim to constrain the radial extent…

astro-ph.SR2016★ 206 cited

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.EP2016★ 617 cited

ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses

Megan Ansdell, Jonathan P. Williams, Nienke van der Marel +12

We present the first high-resolution sub-mm survey of both dust and gas for a large population of protoplanetary disks. Characterizing fundamental properties of protoplanetary disk…

astro-ph.SR2015★ 34 cited

Gas inside the 97 au cavity around the transition disk Sz\,91

H. Canovas, M. R. Schreiber, C. Cáceres +9

We present ALMA (Cycle 0) band-6 and band-3 observations of the transition disk Sz\,91. The disk inclination and position angle are determined to be $i=49.5\degr\pm3.5\degr$ and $\…

astro-ph.SR2014★ 8 cited

Herschel -PACS observations of [OI] and H2O in Cha II

P. Riviere-Marichalar, A. Bayo, I. Kamp +11

Gas plays a major role in the dynamical evolution of protoplanetary discs. Its coupling with the dust is the key to our understanding planetary formation. Studying the gas content…