activity
20142024
most citedA radio pulsing white dwarf binary star

215 citations · 769 across the 25 of their papers we have counts for

collaborators

19 papers

astro-ph.SR202322 cited

Photometric follow-up of 43 new eclipsing white dwarf plus main-sequence binaries from the ZTF survey

Alex J. Brown, Steven G. Parsons, Jan van Roestel +12

Wide-field time-domain photometric sky surveys are now finding hundreds of eclipsing white dwarf plus M dwarf binaries, a population encompassing a wealth of information and potent…

astro-ph.SR202210 cited

Multi-colour optical light curves of the companion star to the millisecond pulsar PSR J2051-0827

V. S. Dhillon, M. R. Kennedy, R. P. Breton +16

We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and…

astro-ph.SR202217 cited

Long-term photometric monitoring and spectroscopy of the white dwarf pulsar AR Scorpii

Ingrid Pelisoli, T. R. Marsh, S. G. Parsons +14

AR Scorpii (AR Sco) is the only radio-pulsing white dwarf known to date. It shows a broad-band spectrum extending from radio to X-rays whose luminosity cannot be explained by therm…

astro-ph.SR202116 cited

The post-common-envelope binary central star of the planetary nebula Ou 5: a doubly-eclipsing post-red-giant-branch system

David Jones, James Munday, Romano Corradi +10

We present a detailed study of the stellar and orbital parameters of the post-common envelope binary central star of the planetary nebula Ou~5. Low-resolution spectra obtained duri…

astro-ph.SR20219 cited

Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4

A. D. Romero, G. R. Lauffer, A. G. Istrate +1

Pulsating low-mass white dwarf stars are white dwarfs with stellar masses between 0.30~M and 0.45~M that show photometric variability due to gravity-mode pulsat…

astro-ph.EP20161 cited

A Circumbinary Debris Disk in a Polluted White Dwarf System

J. Farihi, S. G. Parsons, B. T. Gänsicke

Planetary systems commonly survive the evolution of single stars, as evidenced by terrestrial-like planetesimal debris observed orbiting and polluting the surfaces of white dwarfs.…