collaborators

13 papers

astro-ph.SR2026

Toward 3D orbits of wide sdO/B binaries I. Six composite systems spatially resolved with VLTI/GRAVITY

K. Deshmukh, S. Geier, H. Sana +7

The authors use VLTI/GRAVITY long‑baseline interferometry to spatially resolve six wide hot subdwarf (sdO/B) + main‑sequence binary systems, providing precise separations that will…

astro-ph.IM2026

Studying hot evolved stars with ultraviolet spectroscopy

Stephan Geier, Nicole Reindl, Matti Dorsch +7

Hot evolved stars are key objects to reconstruct the various evolutionary pathways of Sun-like stars, to probe binary interactions and the physics of supernovae. They serve as powe…

astro-ph.SR2026

Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948

M. Pritzkuleit, M. Dorsch, M. M. Miller Bertolami +3

Hot subdwarf stars with masses above ascend the helium giant branch after the end of core helium burning, before entering the white dwarf cooling track or exploding a…

astro-ph.SR2026

Two hot pre-white dwarfs inside the red-giant-branch planetary nebula Pa 13 -- Double core evolution or common envelope-induced rejuvenation?

Nicole Reindl, David Jones, Todd Hillwig +4

Close binary central stars of PNe offer a unique window for investigating the conditions immediately following the ejection of a common envelope (CE). Double eclipsing and double-l…

astro-ph.SR2026

Discovery of a runaway star likely ejected by a Type Iax Supernova

A. Bhat, M. Hollands, M. Dorsch +5

Over the past decade, runaway stars have been identified, believed to originate either as surviving donors of Type Ia supernovae or as partially deflagrated accretors producing Typ…

astro-ph.SR2026

Spectral evolution of hot hybrid white dwarfs: II. Photometry

Semih Filiz, Nicole Reindl, David Jones +4

We present a photometric analysis of 19 DA and 13 DAO white dwarfs (WDs) with effective temperatures exceeding 60 kK, building on the spectral analysis reported in the first paper…