activity
20062025
most citedDo most planetary nebulae derive from binaries? I Population synthesis model of the galactic planetary nebula population produced by singlestars and binaries

136 citations · 300 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2025

Central-star extinctions towards planetary nebulae

Alexander Csukai, Albert A. Zijlstra, Iain McDonald +1

Planetary nebulae trace the hottest and most luminous phase of evolution of solar-type stars. We use these hot, bright stars to investigate extinctions towards a complete sample of…

astro-ph.SR2025

Three-dimensional simulations of accretion disks in pre-CE systems

Ana L. Juarez-Garcia, Orsola De Marco, Fabio De Colle +4

Before a binary system enters into a common envelope (CE) phase, accretion from the primary star onto the companion star through Roche Lobe overflow (RLOF) will lead to the formati…

astro-ph.SR2024

Novel Constraints on Companions to the Helix Nebula Central Star

Leyla Iskandarli, Jay Farihi, Joshua D. Lothringer +3

The Helix is a visually striking and the nearest planetary nebula, yet any companions responsible for its asymmetric morphology have yet to be identified. In 2020, low-amplitude ph…

astro-ph.SR2024

High-Speed Outflows and Dusty Disks during the AGB to PN Transition: The PANORAMA survey

Raghvendra Sahai, Javier Alcolea, Bruce Balick +15

As mass-losing asymptotic giant branch (AGB) stars evolve to planetary nebulae (PNe), the mass outflow geometries transform from nearly spherical to extreme aspherical. The physica…

astro-ph.SR2021★ 37 cited

Binary Central Stars of Planetary Nebulae Identified With Kepler/K2

George H. Jacoby, Todd C. Hillwig, David Jones +6

We present the identification of 34 likely binary central stars (CSs) of planetary nebulae (PNe) from {\it Kepler/K2} data, seven of which show eclipses. Of these, 29 are new disco…

astro-ph.SR2019★ 50 cited

Bipolar Planetary Nebulae from Outflow Collimation by Common Envelope Evolution

Yangyuxin Zou, Adam Frank, Zhuo Chen +8

The morphology of bipolar planetary nebulae (PNe) can be attributed to interactions between a fast wind from the central engine and dense toroidal shaped ejecta left over from comm…