activity
20052026
most citedExtreme helium stars: non-LTE matters Helium and hydrogen spectra of the unique objects V652 Her and HD144941

32 citations · 46 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Evidence for neutron capture in heavy-metal hot subdwarfs: Far-UV spectroscopy of EC22536-5304 and LSIV-14 116

M. Dorsch, C. S. Jeffery, J. Deprince +8

Most hot subdwarfs (sdO/B) are low-mass core-helium-burning stars formed through binary interaction. A subgroup of intermediate He-rich sdOBs shows extreme heavy-metal (Z>30) enric…

astro-ph.SR2026

TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars

Courtney L. Crawford, C. Simon Jeffery, May G. Pedersen +4

Extreme helium stars (EHes) are low-mass hydrogen-deficient stars thought to be the products of double white dwarf mergers. Despite prolonged ground-based observations, there is no…

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.SR2014★ 14 cited

Subaru and Swift observations of V652 Herculis: resolving the photospheric pulsation

C. S. Jeffery, D. Kurtz, H. Shibahashi +4

High resolution spectroscopy with the Subaru High Dispersion Spectrograph, and Swift ultraviolet photometry are presented for the pulsating extreme helium star V652\,Her. Swift pro…

astro-ph.SR2011

Variable Stars

G. Handler, K. R. Pollard, M. S. Cunha +10

This is the triennial report of IAU Commission 27, mostly presenting a review of recent advances in the field.

astro-ph2005★ 32 cited

Extreme helium stars: non-LTE matters Helium and hydrogen spectra of the unique objects V652 Her and HD144941

N. Przybilla, K. Butler, U. Heber +1

Quantitative analyses of low-mass hydrogen-deficient (super-)giant stars - so-called extreme helium stars - to date face two major difficulties. First, theory fails to reproduce th…