activity
20072026
most citedRadio to gamma-ray variability study of blazar S5 0716+714

116 citations · 1.6k across the 50 of their papers we have counts for

collaborators

54 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.IM2026

Probing cold gas and dust in quiescent galaxies across cosmic time

Anita Zanella, Sirio Belli, Belen Alcalde Pampliega +35

The discovery of massive quiescent galaxies at high redshift by JWST has revealed that star formation can cease rapidly in the early Universe, yet the physical mechanisms responsib…

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

The Last Gasps of a Dying Star: ALMA Observations of the Pre-Planetary Nebula IRAS 06530-0213

Raghvendra Sahai, Wouter Vlemmings, Guillermo Quintana-Lacaci +16

We present high angular-resolution () ALMA observations of millimeter-wave line and continuum emission (at and mm) in the pre-planetary ne…

astro-ph.SR2026

The formation radius of HCN in O-rich asymptotic giant branch stars

L. Marinho, J. P. Fonfría, M. Agúndez +3

Molecules detected in circumstellar envelopes around asymptotic giant branch (AGB) stars are generally well explained in terms of formation under chemical equilibrium in the stella…