activity
20122026
most citedThe gravitational-wave signal generated by a galactic population of double neutron-star binaries

26 citations · 83 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

Surface brightness inhomogeneity on the helium-rich hot subdwarf in the X-ray binary HD 49798

C. Simon Jeffery, Gavin Ramsay

HD 49798 is an X-ray binary consisting of a hot helium-rich subdwarf primary and an accreting compact companion with an orbital period of 1.55 d. TESS observations of its optical l…

astro-ph.HE2025

The diverse morphology of gravitational wave signals from merging neutron-star white-dwarf binaries

Shenghua Yu, Youjun Lu, C. Simon Jeffery +6

In sufficiently compact neutron star-white dwarf (NSWD) binary systems, orbital decay means the white dwarf eventually fills its shrinking Roche lobe, initiating a phase of mass tr…

astro-ph.SR2025

Theoretical models for the Late Thermal Pulse in post-AGB stars: the case of DY Cen

Zhongyang Liu, C. Simon Jeffery, Xianfei Zhang +2

We present theoretical predictions of the born-again scenario for post-asymptotic giant-branch stars. An extensive model grid for born-again objects has been constructed, particula…

astro-ph.SR2025

K2 observations of five pulsating subdwarf B stars with white dwarf companions

M. D. Reed, A. S. Baran, J. H. Telting +3

We report seismic analyses of five pulsating subdwarf B (sdBV) stars observed during Kepler's K2 mission, each with a white dwarf companion. We find three of the five to be g-mode-…

astro-ph.SR2025

Linear and non-linear models for large-amplitude radial pulsation in faint blue stars (BLAPs)

C. S. Jeffery

The recent discovery of large-amplitude pulsations in faint blue stars (BLAPs) provides both challenges for stellar pulsation theory and opportunities to explore the late evolution…

astro-ph.SR2024

Spectroscopic diagnostics of lead stratification in hot subdwarf atmospheres

L. J. A. Scott, C. S. Jeffery, C. M. Byrne +1

Heavy metal subdwarfs are a class of hot subdwarfs with very high abundances of heavy elements, typically around 10 000 times solar. They include stars which are strongly enhanced…