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20152026
most citedDust masses of young disks: constraining the initial solid reservoir for planet formation

204 citations · 2.6k across the 110 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR20171 cited

Accretion onto young stars: the key to disk evolution

Carlo F. Manara

The early stages of the pre-Main-Sequence (PMS) evolution of young stars are characterized by a substantial interaction between the central star and the surrounding disk. Among the…

astro-ph.SR201728 cited

Mapping young stellar populations towards Orion with Gaia DR1

E. Zari, A. G. A. Brown, J. de Bruijne +2

We use the first data release of the Gaia mission to explore the three dimensional arrangement and the age ordering of the many stellar groups towards the Orion OB association, aim…

astro-ph.SR2017106 cited

Connection between jets, winds and accretion in T Tauri stars: the X-shooter view

B. Nisini, S. Antoniucci, J. M. Alcala' +5

We have analysed the [OI]6300 A line in a sample of 131 young stars with discs in the Lupus, Chamaeleon and signa Orionis star forming regions, observed with the X-shooter spectrog…

astro-ph.SR201796 cited

Protoplanetary disc `isochrones' and the evolution of discs in the plane

Giuseppe Lodato, Chiara E. Scardoni, Carlo F. Manara +1

In this paper, we compare simple viscous diffusion models for the disc evolution with the results of recent surveys of the properties of young protoplanetary discs. We introduce th…

astro-ph.SR201790 cited

Constraints from Dust Mass and Mass Accretion Rate Measurements on Angular Momentum Transport in Protoplanetary Disks

Gijs D. Mulders, Ilaria Pascucci, Carlo F. Manara +5

We investigate the relation between disk mass and mass accretion rate to constrain the mechanism of angular momentum transport in protoplanetary disks. Dust mass and mass accretion…

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…