activity
20132026
most citedStrongly star-forming rotating disks in a complex merging system at z = 4,7 as revealed by ALMA

81 citations · 277 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Periodic activity on the (sub)mm surface of the AGB star Mira A

M. Andriantsaralaza, B. Bojnordi Arbab, W. Vlemmings +7

Evolved stars on the asymptotic giant branch (AGB) lose mass through stellar winds launched from their dynamic extended atmospheres. Recent high-angular-resolution observations of…

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.SR2023★ 9 cited

Charting Circumstellar Chemistry of Carbon-rich AGB Stars: I. ALMA 3 mm spectral surveys

R. Unnikrishnan, E. De Beck, L. A. Nyman +10

AGB stars are major contributors to the chemical enrichment of the ISM through nucleosynthesis and extensive mass loss. Most of our current knowledge of AGB atmospheric and circums…

astro-ph.SR2021★ 3 cited

Heavy-element Rydberg transition line emission from the post-giant-evolution star HD101584

H. Olofsson, J. H. Black, T. Khouri +7

We report the detection of two lines at millimetre wavelengths towards the immediate surroundings of the post-giant and most likely post-common-envelope star HD101584 using high-an…

astro-ph.SR2020★ 6 cited

VLTI/PIONIER reveals the close environment of the evolved system HD101584

J. Kluska, H. Olofsson, H. Van Winckel +9

Context: The observed orbital characteristics of post-asymptotic giant branch (post-AGB) and post-red giant branch (post-RGB) binaries are not understood. We suspect that the missi…

astro-ph.SR2018★ 34 cited

Rotation of the asymptotic giant branch star R Doradus

W. H. T. Vlemmings, T. Khouri, E. De Beck +7

High resolution observations of the extended atmospheres of asymptotic giant branch (AGB) stars can now directly confront the theories that describe stellar mass loss. Using Atacam…