activity
20232026
most citedClose-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars

58 citations · 104 across the 12 of their papers we have counts for

collaborators
Showing 2025Show all

5 papers · 1 filter

astro-ph.EP2025★ 5 cited

Changing disc compositions via internal photoevaporation II: M dwarf systems

Julia Lena Lienert, Bertram Bitsch, Thomas Henning

The chemical evolution of the inner regions of protoplanetary discs is a complex process. Several factors influence it, one being the inward drift and evaporation of volatile-rich…

astro-ph.EP2025★ 24 cited

Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio

Adrien Houge, Anders Johansen, Edwin Bergin +5

The largest reservoir of carbon in protoplanetary discs is stored in refractory organics, which thermally decompose into the gas-phase at the organics line, well interior to the wa…

astro-ph.EP2025

MINDS. Water reservoirs of compact planet-forming dust disk: A diversity of HO distributions

Milou Temmink, Andrew D. Sellek, Danny Gasman +17

Millimetre-compact dust disks are thought to have efficient radial drift of icy dust pebbles, which has been hypothesised to produce an enhanced cold (400 K) HO reservoir i…

astro-ph.EP2025

Dust processing in the terrestrial planet-forming region of the PDS 70 disk

Yao Liu, Dafa Li, Hongchi Wang +5

Dust grains in protoplanetary disks are the building blocks of planets. Investigating the dust composition and size, and their variation over time, is crucial for understanding the…

astro-ph.EP2025★ 1 cited

MINDS. The influence of outer dust disc structure on the volatile delivery to the inner disc

Danny Gasman, Milou Temmink, Ewine F. van Dishoeck +18

ALMA has revealed that the millimetre dust structures of protoplanetary discs are extremely diverse. It has been proposed that the strength of HO emission in the inner disc par…