activity
20102026
most citedProbing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - II. CO line survey of evolved stars: derivation of mass-loss rate formulae

242 citations · 1.8k across the 49 of their papers we have counts for

collaborators

53 papers

astro-ph.IM2026

Evolved stars: dust formation and mass loss

Luis Velilla-Prieto, Wouter Vlemmings, Guillermo Quintana-Lacaci +18

Evolved stars drive the chemical enrichment of the Universe, acting as primary producers of elemental products of nucleosynthesis and cosmic dust. Unraveling the exact role played…

astro-ph.IM2026

Evolved stars, multiplicity and planets: Shaping and Being Shaped by Stellar Evolution

Theo Khouri, Wouter Vlemmings, Elvire De Beck +21

Understanding how planets and stellar companions survive and interact with their host stars as they evolve, or are ultimately destroyed in the process, is essential both for predic…

astro-ph.SR2026

MATISSE unveils a dusty disc in the interior of EP Aquarii. First evidence of a misaligned hierarchical triple system with a central AGB star?

J. Alonso-Hernández, C. Paladini, C. Sánchez Contreras +26

Aims. We have mapped the dust and molecular gas emission distributions in the vicinity (a few stellar radii) of the asymptotic giant branch (AGB) star EP\,Aquarii, with a previousl…

astro-ph.SR2026

The Molecular Circumstellar Environments of Red Supergiants in Galactic Open Clusters

Mark A. Siebert, Elvire De Beck, Guillermo Quintana-Lacaci +4

We aim to expand the sample of RSGs with direct measurements of circumstellar gas through millimeter observations of two of the largest coeval RSG populations in the Galaxy: the op…

astro-ph.SR2026

A giant magnetic eruption from the asymptotic giant branch star Mira A

W. Vlemmings, M. Andriantsaralaza, B. Bojnordi Arbab +14

Mass loss during the advanced evolutionary stages of low- and intermediate-mass stars is traditionally attributed to dust-driven winds, whereas the influence of magnetic fields rem…

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…