activity
20072023
most citedPhysics of Eclipsing Binaries. V. General Framework for Solving the Inverse Problem

212 citations · 1.6k across the 47 of their papers we have counts for

collaborators

48 papers

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.SR2023★ 4 cited

Post-red-giant-branch Planetary Nebulae

David Jones, Todd Hillwig, Nicole Reindl

Common envelope events have been associated with the formation of a planetary nebulae since its proposition more than forty five years ago. However, until recently there have been…

astro-ph.SR2022★ 12 cited

Searching for the Next Galactic Luminous Red Nova

Harry Addison, Nadejda Blagorodnova, Paul J. Groot +3

Luminous red novae (LRNe) are astrophysical transients believed to be caused by the partial ejection of a binary star's common envelope (CE) and the merger of its components. The f…

astro-ph.SR2021★ 16 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.SR2021★ 205 cited

TESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26

Andrej Prsa, Angela Kochoska, Kyle E. Conroy +44

In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binar…

astro-ph.SR2021★ 8 cited

The Missing Link? Discovery of Pulsations in the Nitrogen-rich PG 1159 Star PG 1144+005

Paulina Sowicka, Gerald Handler, David Jones +1

Up to 98% of all single stars will eventually become white dwarfs - stars that link the history and future evolution of the Galaxy, and whose previous evolution is engraved in thei…