activity
20082026
most citedFurther ALMA observations and detailed modeling of the Red Rectangle

65 citations · 479 across the 51 of their papers we have counts for

collaborators
Showing 2024Show all

7 papers · 1 filter

astro-ph.SR2024★ 4 cited

Jet formation in post-AGB binaries: Confronting cold magnetohydrodynamic disc wind wind models with observations

Toon De Prins, Hans Van Winckel, Jonathan Ferreira +4

Aims: We consider cold self-similar magnetohydrodynamic (MHD) disc wind solutions to describe jets that are launched from the circumcompanion accretion discs in post-AGB binaries.…

physics.ed-ph2024

Teaching the apparent motion of Sun and stars across four European countries

Hans Bekaert, Wim Van Dooren, Hans Van Winckel +7

In the context of the European Erasmus+ project Teaching ASTronomy at the Educational level (TASTE), we investigated the extent to which a learning module at school and a set of ac…

astro-ph.SR2024★ 8 cited

A dynamic view of V Hydrae. Monitoring of a spectroscopic-binary AGB star with an alkaline jet

L. Planquart, A. Jorissen, A. Escorza +2

The well studied carbon star V Hydrae is known to exhibit a complex asymmetric environment made of a dense equatorial wind and high-velocity outflows, hinting at its transition fro…

astro-ph.SR2024★ 21 cited

VELOcities of CEpheids (VELOCE) I. High-precision radial velocities of Cepheids

Richard I. Anderson, Giordano Viviani, Shreeya S. Shetye +27

This first VELOCE data release comprises 18,225 high-precision RV measurements of 258 bona fide classical Cepheids on both hemispheres collected mainly between 2010 and 2022, along…

astro-ph.SR2024★ 6 cited

s-process Enriched Evolved Binaries in the Galaxy and the Magellanic Clouds

Meghna Menon, Devika Kamath, Maksym Mohorian +2

Post-asymptotic giant branch stars (post-AGB) in binary systems, with typical orbital periods between ~100 to ~1000 days, result from a poorly understood interaction that terminate…

astro-ph.SR2024

The first measurements of carbon isotopic ratios in post-RGB stars: SZ Mon and DF Cyg. E-iSpec: A spectral analysis tool to derive elemental abundances and isotopic ratios for evolved stars

Maksym Mohorian, Devika Kamath, Meghna Menon +4

Dusty post-red giant branch (post-RGB) stars are low- and intermediate-mass stars where the RGB evolution was prematurely terminated by a poorly understood binary interaction. Thes…