activity
20032026
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 · 1.9k across the 47 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.SR2016★ 10 cited

ALMA Compact Array observations of the Fried Egg nebula: Evidence for large-scale asymmetric mass-loss from the yellow hypergiant IRAS 17163-3907

Sofia Wallstrom, E. Lagadec, S. Muller +12

Yellow hypergiants are rare and represent a fast evolutionary stage of massive evolved stars. That evolutionary phase is characterised by a very intense mass loss, the understandin…

astro-ph.SR2016★ 27 cited

The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

M. A. T. Groenewegen, W. H. T. Vlemmings, P. Marigo +21

Context: Low- and intermediate-mass stars lose most of their stellar mass at the end of their lives on the asymptotic giant branch (AGB). Determining gas and dust mass-loss rates (…

astro-ph.SR2016★ 14 cited

Herschel/HIFI observations of the circumstellar ammonia lines in IRC+10216

M. R. Schmidt, J. H. He, R. Szczerba +14

New high-resolution far-infrared (FIR) observations of both ortho- and para-NH3 transitions toward IRC+10216 were obtained with Herschel, with the goal of determining the ammonia a…

astro-ph.SR2016★ 59 cited

A HIFI view on circumstellar H2O in M-type AGB stars: radiative transfer, velocity profiles, and H2O line cooling

M. Maercker, T. Danilovich, H. Olofsson +4

We aim to constrain the temperature and velocity structures, and H2O abundances in the winds of a sample of M-type AGB stars. We further aim to determine the effect of H2O line coo…

astro-ph.SR2016★ 63 cited

Sulphur molecules in the circumstellar envelopes of M-type AGB stars

Taissa Danilovich, E. De Beck, J. H. Black +2

The sulphur compounds SO and SO have not been widely studied in the circumstellar envelopes of asymptotic giant branch (AGB) stars. By presenting and modelling a large number o…