activity
20162024
most citedA radio pulsing white dwarf binary star

215 citations · 290 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

ASASSN-14dx: A cataclysmic variable harbouring a massive pulsating white dwarf

Pasi Hakala, Ingrid Pelisoli, Boris T. Gaensicke +5

We present the results of our study of ASASSN-14dx, a previously known but poorly characterised cataclysmic variable (CV). The source was observed as part of an ongoing high-time-r…

astro-ph.HE20241 cited

Cataclysmic Variables and AM CVn Binaries in SRG/eROSITA + Gaia: Volume Limited Samples, X-ray Luminosity Functions, and Space Densities

Antonio C. Rodriguez, Kareem El-Badry, Valery Suleimanov +22

We present volume-limited samples of cataclysmic variables (CVs) and AM CVn binaries jointly selected from SRG/eROSITA eRASS1 and \textit{Gaia} DR3 using an X-ray + optical color-c…

astro-ph.IM202412 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.SR20232 cited

Structure of the accretion flow of IX Velorum as revealed by high-resolution spectroscopy

Jan Kára, Linda Schmidtobreick, Anna Francesca Pala +1

Context: Several high-mass transfer cataclysmic variables show evidence for outflow from the system, which could play an important role in their evolution. We investigate the syste…

astro-ph.SR20238 cited

Accurate mass-radius ratios for Hyades white dwarfs

L. Pasquini, A. F. Pala, M. Salaris +4

We use the ESPRESSO spectrograph at the Very Large Telescope to measure velocity shifts and gravitational redshifts of eight bona fide Hyades white dwarfs, with an accuracy better…

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…