activity
20202026
most citedMINDS. The detection of CO with JWST-MIRI indicates abundant CO in a protoplanetary disk

109 citations · 1.6k across the 83 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.EP2021★ 28 cited

Effect of MHD wind-driven disk evolution on the observed sizes of protoplanetary disks

Leon Trapman, Benoit Tabone, Giovanni Rosotti +1

It is still unclear whether the evolution of protoplanetary disks, a key ingredient in the theory of planet formation, is driven by viscous turbulence or magnetic disk winds. As vi…

astro-ph.EP2021

MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus

Benoît Tabone, Giovanni P. Rosotti, Giuseppe Lodato +3

The final architecture of planetary systems depends on the extraction of angular momentum and mass-loss processes of the discs in which they form. Theoretical studies proposed that…

astro-ph.SR2021★ 1 cited

Secular evolution of MHD wind-driven discs: analytical solutions in the expanded α-framework

Benoît Tabone, Giovanni P. Rosotti, Alexander J. Cridland +2

The evolution of protoplanetary discs and the related process of planet formation is regulated by angular momentum transport and mass-loss processes. Over the past decade, the para…

astro-ph.EP2021★ 39 cited

Molecules with ALMA at Planet-forming Scales (MAPS) XVI: Characterizing the impact of the molecular wind on the evolution of the HD 163296 system

Alice S. Booth, Benoit Tabone, John D. Ilee +26

During the main phase of evolution of a protoplanetary disk, accretion regulates the inner-disk properties, such as the temperature and mass distribution, and in turn, the physical…

astro-ph.GA2021★ 69 cited

Complex organic molecules in low-mass protostars on Solar System scales -- II. Nitrogen-bearing species

P. Nazari, M. L. van Gelder, E. F. van Dishoeck +10

The chemical inventory of planets is determined by the physical and chemical processes that govern the early phases of star formation. The aim is to investigate N-bearing complex o…

astro-ph.GA2021★ 59 cited

OH mid-infrared emission as a diagnostic of HO UV photodissociation. I. Model and application to the HH 211 shock

Benoît Tabone, Marc C. van Hemert, Ewine F. van Dishoeck +1

Water is an important molecule in interstellar and circumstellar environments. Previous observations of mid-infrared rotational lines of OH suggest that these lines may be used to…