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20222025
most citedATOMIUM: Continuum emission and evidence of dust enhancement from binary motion

7 citations · 23 across the 8 of their papers we have counts for

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astro-ph.SR2025★ 5 cited

Evidence for the Keplerian orbit of a close companion around a giant star

Mats Esseldeurs, Leen Decin, Joris De Ridder +31

Close companions influence stellar evolution through tidal interactions, mass transfer, and mass loss effects. While such companions are detected around young stellar objects, main…

astro-ph.SR2025★ 6 cited

Eppur si eclissa: Eccentric low-mass companions and time-in-dust selection explain long secondary periods

Leen Decin, Owen Vermeulen, Mats Esseldeurs +5

[abbreviated] Long Secondary Periods (LSPs) are observed in about one third of pulsating red giants yet remain unexplained. Four key observational constraints anchor the discussion…

astro-ph.SR2025★ 1 cited

Impact of a binary companion in AGB outflows on CO spectral lines

Owen Vermeulen, Mats Esseldeurs, Jolien Malfait +7

In the late stage of their evolution, low- to intermediate-mass stars pass through the asymptotic giant branch (AGB) phase, characterised by strong mass loss through dust driven wi…

astro-ph.SR2025★ 7 cited

ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion

T. Danilovich, N. Samaratunge, Y. Mori +35

Low- and intermediate-mass stars on the asymptotic giant branch (AGB) account for a significant portion of the dust and chemical enrichment in their host galaxy. Here we present AL…

astro-ph.SR2024

The Effect of Donor Star Rejuvenation on Common Envelope Evolution

C. Landri, P. M. Ricker, M. Renzo +2

In close binary star systems, common envelope evolution may occur after a previous phase of mass transfer. Some isolated formation channels for double neutron star binaries suggest…

astro-ph.SR2024

Driving asymmetric red supergiants winds with binary interactions

Camille Landri, Ondřej Pejcha

Massive stars in the red supergiant (RSG) phase are known to undergo strong mass loss through winds and observations indicate that a substantial part of this mass loss could be dri…