activity
20162024
most citedA radio pulsing white dwarf binary star

215 citations · 243 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20242 cited

The white dwarf binary pathways survey -- X. Gaia orbits for known UV excess binaries

J. A. Garbutt, S. G. Parsons, O. Toloza +9

White dwarfs with a F, G or K type companion represent the last common ancestor for a plethora of exotic systems throughout the galaxy, though to this point very few of them have b…

astro-ph.SR2024

Rotation plays a role in the generation of magnetic fields in single white dwarfs

Mercedes S. Hernandez, Matthias R. Schreiber, John D. Landstreet +5

Recent surveys of close white dwarf binaries as well as single white dwarfs have provided evidence for the late appearance of magnetic fields in white dwarfs, and a possible genera…

astro-ph.SR2023

Asteroseismological analysis of the polluted ZZ Ceti star G29-38 with TESS

Murat Uzundag, Francisco C. De Gerónimo, Alejandro H. Córsico +15

G\,2938 (TIC~422526868) is one of the brightest () and closest (\,pc) pulsating white dwarfs with a hydrogen-rich atmosphere (DAV/ZZ Ceti class). It was obser…

astro-ph.SR2023

An HST COS ultra-violet spectroscopic survey of 311 DA white dwarfs.I. Fundamental parameters and comparative studies

Snehalata Sahu, Boris T. Gaensicke, Pier-Emmanuel Tremblay +8

White dwarf studies carry significant implications across multiple fields of astrophysics, including exoplanets, supernova explosions, and cosmological investigations. Thus, accura…

astro-ph.SR202316 cited

Systematic uncertainties in the characterisation of helium-dominated metal-polluted white dwarf atmospheres

Paula Izquierdo, Boris T. Gänsicke, Pablo Rodríguez-Gil +5

White dwarf photospheric parameters are usually obtained by means of spectroscopic or photometric analysis. These results are not always consistent with each other, with the publis…

astro-ph.SR202210 cited

Testing Lyman alpha emission line reconstruction routines at multiple velocities in one system

David J. Wilson, Allison Youngblood, Odette Toloza +6

The 1215.67A HI Lyman alpha emission line dominates the ultraviolet flux of low mass stars, including the majority of known exoplanet hosts. Unfortunately, strong attenuation by th…