collaborators

6 papers

astro-ph.SR2026

Population synthesis of substellar companions surviving common-envelope evolution

Nicolas F. Miranda, Alex Mauch-Soriano, Joaquin A. Barraza-Jorquera +3

Predicting the population of substellar companions around white dwarfs (WDs) requires accounting for both companions that avoid engulfment during stellar evolution and those that s…

astro-ph.SR2026

A double debris disc around a white dwarf sculpted by two planetary bodies

Nicola Pietro Gentile Fusillo, Felipe Lagos-Vilches, Boris T. Gänsicke +2

Many planetary systems survive the metamorphosis of their hosts stars into white dwarfs, as demonstrated by the detection of dusty circumstellar discs around these stellar remnants…

astro-ph.SR2026

The white dwarf binary pathways survey - XI. The Gaia-GALEX UV Excess Sample for systems within 350 pc

James A. Garbutt, S. G. Parsons, N. Gentile Fusillo +9

White dwarfs (WDs) with F, G or K type binary companions are the last common ancestor to a zoo of exotic phenomena. Finding a clean sample of such systems is difficult, as WDs in s…

astro-ph.SR2026

Direct detections of white dwarfs in four WD+dM post-common envelope binaries within 20 pc

Mairi W. O'Brien, David J. Wilson, Pier-Emmanuel Tremblay +5

Characterising post-common envelope binaries (PCEBs) containing a white dwarf and a main-sequence companion is essential for improving theories of binary evolution. This paper pres…

astro-ph.EP2026

Predicted incidence of Jupiter-like planets around white dwarfs

Alex Mauch-Soriano, Matthias R. Schreiber, Diego Correa +7

Only a handful of gas giant planets orbiting white dwarfs are known. It remains unclear whether this paucity reflects observational challenges or the consequences of stellar evolut…

astro-ph.SR2024

Most extremely low mass white dwarfs with non-degenerate companions are inner binaries of hierarchical triples

Felipe Lagos-Vilches, Mercedes Hernandez, Matthias R. Schreiber +2

Extremely-low-mass white dwarfs (ELM WDs) with non-degenerate companions are believed to originate from solar-type main-sequence binaries undergoing stable Roche lobe overflow mass…