activity
20092026
most citedThe fastest unbound star in our Galaxy ejected by a thermonuclear supernova

132 citations · 1.1k across the 41 of their papers we have counts for

collaborators

41 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

Hot subdwarf stars (sdO/Bs) are widely considered to be products of binary evolution. A significant fraction of them are found in long-period or wide binaries ( d) with main…

astro-ph.SR2026

The massive hot subdwarf binary LAMOST J065816.72+094343.1

F. Mattig, B. N. Barlow, D. Liu +9

Massive short-period binaries involving hot subdwarf stars (sdO/Bs) are rare but important to constraining pathways for binary star evolution. Moreover, some of the most promising…

astro-ph.IM2026

Experiments in binary evolution

Stephan Geier, Thomas Kupfer, Pierre Maxted +1

The majority of stars more massive than the Sun is found in binary or multiple star systems and many of them will interact during their evolution. Specific interactions, where prog…

astro-ph.SR2024★ 11 cited

A spectroscopic and kinematic survey of fast hot subdwarfs

S. Geier, U. Heber, A. Irrgang +19

Hot subdwarfs (sdO/B) are the stripped helium cores of red giants formed by binary interactions. Close hot subdwarf binaries with massive white dwarf companions have been proposed…

astro-ph.SR2024

A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties

H. Dawson, S. Geier, U. Heber +25

We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the {\em Gaia}…

astro-ph.SR2023★ 21 cited

Hot subdwarfs in close binaries observed from space II: Analysis of the light curves

V. Schaffenroth, B. N. Barlow, I. Pelisoli +2

Hot subdwarfs in close binaries with either M dwarf, brown dwarf or white dwarf companions show unique light variations. In hot subdwarf binaries with M dwarf or brown dwarf compan…