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20172020
most citedRings and filaments: The remarkable detached CO shell of U Antliae

23 citations · 46 across the 3 of their papers we have counts for

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astro-ph.SR2020★ 2 cited

Extended view on the dust shells around two carbon stars

M. Mečina, B. Aringer, W. Nowotny +4

Stars on the asymptotic giant branch (AGB) lose considerable amounts of matter through their dust-driven stellar winds. A number of such sources have been imaged by Herschel/PACS,…

astro-ph.SR2018

ALMA observations of the "fresh" carbon-rich AGB star TX Piscium. The discovery of an elliptical detached shell

Magdalena Brunner, Marko Mecina, Matthias Maercker +4

Aims. The carbon-rich asymptotic giant branch (AGB) star TX Piscium (TX Psc) has been observed multiple times during multiple epochs and at different wavelengths and resolutions, s…

astro-ph.SR2018

Properties of dust in the detached shells around U Ant, DR Ser, and V644 Sco

M. Maercker, T. Khouri Silva, E. De Beck +3

Understanding the properties of dust produced during the asymptotic giant branch phase of stellar evolution is important for understanding the evolution of stars and galaxies. Rece…

astro-ph.SR2018

Molecular line study of the S-type AGB star W Aquilae. ALMA observations of CS, SiS, SiO and HCN

Magdalena Brunner, Taissa Danilovich, Sofia Ramstedt +5

Context. With the outstanding spatial resolution and sensitivity of the Atacama Large Millimeter/sub-millimeter Array (ALMA), molecular gas other than the abundant CO can be observ…

astro-ph.SR2017★ 21 cited

The circumstellar envelope around the S-type AGB star W Aql Effects of an eccentric binary orbit

S. Ramstedt, S. Mohamed, W. H. T. Vlemmings +9

The CO(J=3-2) emission from the CSE of the binary S-type AGB star W Aql has been observed at subarcsecond resolution using ALMA. The aim of this paper is to investigate the wind pr…

astro-ph.SR2017★ 23 cited

Rings and filaments: The remarkable detached CO shell of U Antliae

F. Kerschbaum, M. Maercker, M. Brunner +11

Aims. Our goal is to characterize the intermediate age, detached shell carbon star U Antliae morphologically and physically in order to study the mass-loss evolution after a possib…