activity
20222026
most citedJWST detection of heavy neutron capture elements in a compact object merger

230 citations · 324 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

Circular polarimetry of suspect wind-accreting pre-polars II

Pasi Hakala, Steven Parsons, Gavin Ramsay +2

The origin of white dwarf magnetic fields is an open question. Furthermore, such fields play a vital role in the evolution of interacting binary stars. Here we present a study of w…

astro-ph.SR2026

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories

James Munday, Antonio C. Rodriguez, Nicole Reindl +23

The AM CVn class includes mass transferring, ultra-compact double white dwarf binaries with orbital periods on the timescale of minutes. A long-standing puzzle is that none of the…

astro-ph.SR2026

No Period Change in Two Long-Period AM CVn Binaries

Matthew J. Green, Thomas R. Marsh, Jan van Roestel +25

Ultracompact binary systems, consisting of two compact objects in an orbit , should exhibit measurable rates of orbital period change () due t…

astro-ph.SR2026

An eclipsing 8.56 minute orbital period mass-transferring binary

Emma T. Chickles, Joheen Chakraborty, Kevin B. Burdge +34

We report the discovery of ATLAS J101342.5-451656.8 (hereafter ATLAS J1013-4516), an 8.56 minute orbital period mass transferring AM Canum Venaticorum binary with mean Gaia magnitu…

astro-ph.SR2024

A gravitational wave detectable candidate Type Ia supernova progenitor

Emma T. Chickles, Kevin B. Burdge, Joheen Chakraborty +37

Type Ia supernovae, critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear. Growing evide…

astro-ph.HE2024

Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks

Joheen Chakraborty, Kevin B. Burdge, Saul A. Rappaport +35

We report the discovery of three ultracompact binary white dwarf systems hosting accretion disks, with orbital periods of 7.95, 8.68, and 13.15 minutes. This significantly augments…

astro-ph.SR2024

The double low-mass white dwarf eclipsing binary system J2102-4145 and its possible evolution

Larissa Antunes Amaral, James Munday, Maja Vučković +7

Approximately 150 low-mass white dwarfs, with masses below 0.4Msun, have been discovered. The majority of these low-mass WDs are observed in binary systems as they cannot be formed…

astro-ph.SR2023

TIC 378898110: A Bright, Short-Period AM CVn Binary in TESS

Matthew J. Green, J. J. Hermes, Brad N. Barlow +22

AM CVn-type systems are ultracompact, helium-accreting binary systems which are evolutionarily linked to the progenitors of thermonuclear supernovae and are expected to be strong G…

astro-ph.SR2023★ 17 cited

A rotating white dwarf shows different compositions on its opposite faces

Ilaria Caiazzo, Kevin B. Burdge, Pier-Emmanuel Tremblay +35

White dwarfs, the extremely dense remnants left behind by most stars after their death, are characterised by a mass comparable to that of the Sun compressed into the size of an Ear…

astro-ph.SR2023★ 10 cited

An Eclipsing 47 minute Double White Dwarf Binary at 400 pc

James Munday, P. -E. Tremblay, J. J. Hermes +20

We present the discovery of the eclipsing double white dwarf (WD) binary WDJ 022558.21-692025.38 that has an orbital period of 47.19 min. Following identification with the Transiti…

astro-ph.HE2023★ 230 cited

JWST detection of heavy neutron capture elements in a compact object merger

A. Levan, B. P. Gompertz, O. S. Salafia +80

The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray burs…

astro-ph.SR2023★ 22 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.SR2022★ 24 cited

Two decades of optical timing of the shortest-period binary star system HM Cancri

James Munday, T. R. Marsh, Mark Hollands +15

The shortest-period binary star system known to date, RX J0806.3+1527 (HM Cancri), has now been observed in the optical for more than two decades. Although it is thought to be a do…

astro-ph.SR2022★ 21 cited

Characterising eclipsing white dwarf M dwarf binaries from multi-band eclipse photometry

Alex J. Brown, Steven G. Parsons, Stuart P. Littlefair +10

With the prevalence of wide-field, time-domain photometric sky surveys, the number of eclipsing white dwarf systems being discovered is increasing dramatically. An efficient method…