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20102026
most cited(Sub)stellar companions shape the winds of evolved stars

132 citations · 1.2k across the 58 of their papers we have counts for

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Showing 2021Show all

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astro-ph.SR2021★ 26 cited

Observational identification of a sample of likely recent Common-Envelope Events

Theo Khouri, Wouter Vlemmings, Daniel Tafoya +5

One of the most poorly understood stellar evolutionary paths is that of binary systems undergoing common-envelope evolution, when the envelope of a giant star engulfs the orbit of…

astro-ph.SR2021★ 38 cited

ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars: Motivation, sample, calibration, and initial results

C. A. Gottlieb, L. Decin, A. M. S. Richards +33

This overview paper presents ATOMIUM, a Large Programme in Cycle 6 with the Atacama Large Millimeter-submillimeter Array (ALMA). The goal of ATOMIUM is to understand the dynamics a…

astro-ph.SR2021★ 7 cited

Maser emission from the CO envelope of the asymptotic giant branch star W Hydrae

W. H. T. Vlemmings, T. Khouri, D. Tafoya

Observation of CO emission around asymptotic giant branch (AGB) stars is the primary method to determine gas mass-loss rates. While radiative transfer models have shown that molecu…

astro-ph.SR2021★ 21 cited

ATOMIUM: Halide molecules around the S-type AGB star W Aquilae

T. Danilovich, M. Van de Sande, J. M. C. Plane +36

S-type asymptotic giant branch (AGB) stars are thought to be intermediates in the evolution of oxygen- to carbon-rich AGB stars. The chemical compositions of their circumstellar en…

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

SiO masers and 7 mm Continuum in Mira and R Aqr

W. D. Cotton, E. Humphreys, M. Wittkowski +5

Interactions between AGB stars and a secondary in a close orbit are one possible explanation of why some AGB stars develop into aspherical planetary nebulae. This study uses millim…

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…