activity
20242026
most citedJOYS: Linking the molecular ice and gas-phase composition towards the high-mass hot core IRAS 18089-1732

2 citations · 2 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2026

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties

Pacôme Estève, Benoît Tabone, Emilie Habart +5

(Abridged) We aim to explore the parameters that influence the mid-infrared emission of CH and HO, and if the spread observed in / is tr…

astro-ph.EP2025

Vertical CO surfaces as a probe for protoplanetary disk mass and carbon depletion

T. Paneque-Carreño, A. Miotello, E. F. van Dishoeck +2

As the sample of mid-inclination disks with measured CO emission surfaces grows, a fundamental unanswered question is how these vertical profiles connect to their host properties.…

astro-ph.EP2024

A complete Herbig disk mass survey in Orion

L. M. Stapper, M. R. Hogerheijde, E. F. van Dishoeck +3

Disks around intermediate mass stars called Herbig disks are the formation sites of giant exoplanets. Obtaining a complete inventory of these disks will therefore give insights int…

astro-ph.EP2024

Intermediate mass T Tauri disk masses and a comparison to their Herbig disk descendants

L. M. Stapper, M. R. Hogerheijde, E. F. van Dishoeck +3

The precursors of Herbig stars are called Intermediate Mass T Tauri (IMTT) stars, which have spectral types later than F, but stellar masses between 1.5 and 5 M_\odot, and will eve…

astro-ph.EP2024

Chemistry across dust and gas gaps in protoplanetary disks: modelling the co-spatial molecular rings in the HD 100546 disk

M. Leemker, A. S. Booth, E. F. van Dishoeck +2

High-resolution observations show that typically both the dust and the gas in nearby extended protoplanetary disks are structured, possibly related to radial and azimuthal variatio…