activity
20222026
most citedThe structure of jets launched from post-AGB binary systems

28 citations · 114 across the 16 of their papers we have counts for

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Showing 2024Show all

8 papers · 1 filter

astro-ph.SR2024

X-Shooting ULLYSES: Massive stars at low metallicity VI. Atmosphere and mass-loss properties of O-type giants in the Small Magellanic Cloud

Frank Backs, S. A. Brands, A. de Koter +21

Mass loss through a stellar wind is an important physical process that steers the evolution of massive stars and controls the properties of their end-of-life products, such as the…

astro-ph.SR2024★ 20 cited

X-Shooting ULLYSES: Massive Stars at low metallicity IX: Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud

O. Verhamme, J. Sundqvist, A. de Koter +16

Context. Current implementations of mass loss for hot, massive stars in stellar evolution models include a sharp increase in mass loss when blue supergiants become cooler than Teff…

astro-ph.SR2024

X-Shooting ULLYSES: Massive stars at low metallicity VII. Stellar and wind properties of B supergiants in the Small Magellanic Cloud

M. Bernini-Peron, A. A. C. Sander, V. Ramachandran +22

Context. B supergiants (BSGs) represent an important connection between the main sequence and more extreme evolutionary stages of massive stars. Additionally, lying toward the cool…

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.…

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★ 22 cited

X-Shooting ULLYSES: Massive Stars at low metallicity II. DR1: Advanced optical data products for the Magellanic Clouds

H. Sana, F. Tramper, M. Abdul-Masih +34

Using the medium resolution spectrograph X-shooter, spectra of 235 OB and Wolf-Rayet (WR) stars in sub-solar metallicity environments have been secured. [...]This second paper focu…

astro-ph.SR2024

2D unified atmosphere and wind simulations of O-type stars

D. Debnath, J. O. Sundqvist, N. Moens +3

Massive and luminous O-star atmospheres with winds have been studied primarily using one-dimensional (1D), spherically symmetric, and stationary models. However, observations and t…

astro-ph.SR2024★ 8 cited

Magnetically driven winds from accretion disks in post-asymptotic giant branch binaries

Olivier Verhamme, Jacques Kluska, Jonathan Ferreira +4

Context. Jets are commonly detected in post-asymptotic giant branch (post-AGB) binaries and originate from an accretion process onto the companion of the post-AGB primary. These je…