activity
20022026
most citedA far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants

202 citations · 2.2k across the 51 of their papers we have counts for

collaborators

53 papers

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

CO rotational line emission in very red carbon stars in the Magellanic Clouds

M. A. T. Groenewegen, A. Nanni, M. L. Boyer +11

Stars of low and intermediate initial mass lose most of their stellar mass at the end of their lives during the asymptotic giant branch (AGB) phase. Determining their gas and dust…

astro-ph.SR2025★ 1 cited

X TrA through the eyes of MATISSE: More evidence of clumpy molecular layers around C-type asymptotic giant branch stars

V. Răstău, C. Paladini, J. Drevon +22

Aims. The goal of this study is to further the understanding of the wind formation mechanism in asymptotic giant branch (AGB) stars through the analysis of the close environment (w…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2024★ 3 cited

Probing the dynamical and kinematical structures of detached shells around AGB stars

M. Maercker, E. De Beck, T. Khouri +6

Aims. We aim to resolve the spatial and kinematic sub-structures in five detached-shell sources to provide detailed constraints for hydrodynamic models that describe the formation…

astro-ph.SR2023★ 3 cited

Extended far-UV emission surrounding asymptotic giant branch stars as seen by GALEX

V. Răstău, M. Mečina, F. Kerschbaum +5

Aims. Our goal is to study the long-term mass-loss rate characteristics of asymptotic giant branch (AGB) stars through wind-wind and wind-interstellar medium interaction. Methods.…