collaborators

4 papers

astro-ph.SR2026

OH/IR stars in the inner Galactic bulge: I. Colour, CO line, and stellar light curve characteristics

H. Olofsson, T. Khouri, S. Muller +11

Stars on the asymptotic giant branch (AGB) play important roles in a number of astronomical contexts. To quantify these roles, it is necessary to establish the mass-loss characteri…

astro-ph.SR2026

Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. III. SiO and SiS abundances

R. Unnikrishnan, E. De Beck, L. -Ã . Nyman +9

The present understanding of C-rich AGB chemistry largely relies on observations of the archetypal carbon star IRC+10216. Current molecular abundance estimates for carbon stars are…

astro-ph.SR2025

An empirical view of the extended atmosphere and inner envelope of the asymptotic giant branch star R Doradus. II. Constraining the dust properties with radiative transfer modelling

Thiebaut Schirmer, Theo Khouri, Wouter Vlemmings +6

Mass loss in oxygen-rich asymptotic giant branch (AGB) stars remains poorly understood, as the dust detected around them appears too transparent to drive winds through absorption a…

astro-ph.SR2025

Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. II. Abundances and spatial distributions of CS

R. Unnikrishnan, M. Andriantsaralaza, E. De Beck +9

The circumstellar envelopes (CSEs) of asymptotic giant branch (AGB) stars harbour a rich variety of molecules and are sites of complex chemistry. Our current understanding of the c…