activity
20182026
most citedDust-gas chemistry in AGB outflows: Chemical modelling of dust-gas chemistry within AGB outflows I. Effect on the gas-phase chemistry

25 citations · 81 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

ATOMIUM: Inner circumstellar envelopes of oxygen-rich AGB stars as revealed by highly excited SiO lines

B. Pimpanuwat, S. Etoka, M. D. Gray +14

Silicon monoxide (SiO) traces the physical conditions and dynamics in the circumstellar envelopes (CSEs) of AGB stars. We present high-resolution ALMA Band 6 observations of highly…

astro-ph.SR2026

A rotational line CO cooling rate prescription for AGB outflows

T. Ceulemans, F. De Ceuster, O. Vermeulen +1

Asymptotic Giant Branch (AGB) stars significantly contribute to the chemical composition of the universe. In their outflows, complex chemistry takes place, which critically depends…

astro-ph.SR2025★ 7 cited

ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion

T. Danilovich, N. Samaratunge, Y. Mori +35

Low- and intermediate-mass stars on the asymptotic giant branch (AGB) account for a significant portion of the dust and chemical enrichment in their host galaxy. Here we present AL…

astro-ph.GA2023★ 6 cited

Sensitivity study of chemistry in AGB outflows using chemical kinetics

S. Maes, M. Van de Sande, T. Danilovich +2

Asymptotic Giant Branch (AGB) stars shed a significant amount of their mass in the form of a stellar wind, creating a vast circumstellar envelope (CSE). Owing to the ideal combinat…

astro-ph.SR2023★ 10 cited

The unusual 3D distribution of NaCl around the AGB star IK Tau

A. Coenegrachts, T. Danilovich, F. De Ceuster +1

NaCl is a diatomic molecule with a large dipole moment, which allows for its detection even at relatively small abundances. It has been detected towards several evolved stars, amon…

astro-ph.SR2020★ 8 cited

How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions -- The case of EP Aqr

J. Wiegert, M. A. T. Groenewegen, A. Jorissen +2

High-angular-resolution observations of asymptotic giant branch (AGB) stars often reveal non-spherical morphologies for the gas and dust envelopes. We aim to make a pilot study to…

astro-ph.SR2019★ 25 cited

Dust-gas chemistry in AGB outflows: Chemical modelling of dust-gas chemistry within AGB outflows I. Effect on the gas-phase chemistry

M. Van de Sande, C. Walsh, T. P. Mangan +1

Chemical modelling of AGB outflows is typically focused on either non-thermodynamic equilibrium chemistry in the inner region or photon-driven chemistry in the outer region. We inc…

astro-ph.SR2018★ 25 cited

Constraints on metal oxide and metal hydroxide abundances in the winds of AGB stars - Potential detection of FeO in R Dor

L. Decin, T. Danilovich, D. Gobrecht +4

Using ALMA, we observed the stellar wind of two oxygen-rich Asymptotic Giant Branch (AGB) stars, IK Tau and R Dor, between 335 and 362 GHz. One aim was to detect metal oxides and m…