activity
19992023
most citedThe catalogue of radial velocity variable hot subluminous stars from the MUCHFUSS project

65 citations · 372 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2023★ 1 cited

The fastest hot subdwarfs revisited

Ulrich Heber

Hyper-velocity stars (HVS) are enigmatic objects because they are travelling so fast that they escape from the Galaxy. Among hot subdwarfs, only one such star is known, the He-sdO…

astro-ph.SR2022★ 18 cited

The OmegaWhite Survey for Short-Period Variable Stars VII: High amplitude, short period blue variables

G. Ramsay, P. A. Woudt, T. Kupfer +11

Blue Large Amplitude Pulsators (BLAPs) are a relatively new class of blue variable stars showing periodic variations in their light curves with periods shorter than a few tens of m…

astro-ph.SR2022★ 18 cited

The origin of early-type runaway stars from open clusters

Aakash Bhat, Andreas Irrgang, Ulrich Heber

Runaway stars are ejected from their place of birth in the Galactic disk, with some young B-type runaways found several tens of kiloparsecs from the plane traveling at speeds beyon…

astro-ph.SR2021★ 35 cited

Kinematic properties of white dwarfs. Galactic orbital parameters and age-velocity dispersion relation

R. Raddi, S. Torres, A. Rebassa-Mansergas +9

We present the first detailed 3D kinematic analysis of a sample of 3133 white dwarfs that use Gaia astrometry plus radial velocities, which were measured either by Gaia or by groun…

astro-ph.SR2021★ 38 cited

Discovery of a double detonation thermonuclear supernova progenitor

Thomas Kupfer, Evan B. Bauer, Jan van Roestel +12

We present the discovery of a new double detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with an P=76.34179(2) min orbital per…

astro-ph.SR2020★ 22 cited

Heavy-metal enrichment of intermediate He-sdOB stars: the pulsators Feige 46 and LS IV -14 116 revisited

M. Dorsch, M. Latour, U. Heber +3

Hot subdwarf stars of types O and B represent a poorly understood phase in the evolution of low-mass stars. Many subdwarfs show rich oscillations and are among the most chemically…