activity
20072024
most citedA detailed view of the gas shell around R Sculptoris with ALMA

33 citations · 104 across the 9 of their papers we have counts for

collaborators

9 papers

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.SR2021★ 12 cited

DEATHSTAR: Nearby AGB stars with the Atacama Compact Array II. CO envelope sizes and asymmetries: The S-type stars

M. Andriantsaralaza, S. Ramstedt, W. H. T. Vlemmings +13

We aim to constrain the sizes of the CO circumstellar envelopes (CSEs) of 16 S-type stars, along with an additional 7 and 4 CSEs of C-type and M-type AGB stars, respectively. We ma…

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.SR2020

DEATHSTAR: Nearby AGB stars with the Atacama Compact Array I. CO envelope sizes and asymmetries: A new hope for accurate mass-loss-rate estimates

S. Ramstedt, W. H. T. Vlemmings, L. Doan +16

This is the first publication of the DEATHSTAR project. The goal of the project is to reduce the uncertainties of observational estimates of mass-loss rates from Asymptotic Giant B…

astro-ph.SR2015★ 33 cited

A detailed view of the gas shell around R Sculptoris with ALMA

M. Maercker, W. H. T. Vlemmings, M. Brunner +6

Thermal pulses are fundamental to the chemical evolution of AGB stars and their circumstellar envelopes. A further consequence of thermal pulses is the formation of detached shells…