most citedA super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr

8 citations · 17 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2025

The Future of Evolved Planetary Systems

Roberto Raddi, Anna F. Pala, Alberto Rebassa-Mansergas +19

Understanding the formation, evolution, and chemical diversity of exoplanets are now central areas of astrophysics research. White dwarfs provide a uniquely sensitive laboratory fo…

astro-ph.IM2025

The Galactic White Dwarf Population

Santiago Torres, Roberto Raddi, Alberto Rebassa-Mansergas +15

The ESA Gaia mission has revolutionized our understanding of the white dwarf population, delivering an unprecedented census of these nearby remnants and revealing previously unseen…

astro-ph.SR2025

Re-evaluating Lyman wing opacities and the low mass-problem in cool white dwarfs

Snehalata Sahu, Pier-Emmanuel Tremblay, Detlev Koester +4

Gaia observations have reignited interest in the optical and ultraviolet (UV) opacity problems of cool white dwarfs ( K), which were thought to be resolved n…

astro-ph.EP20254 cited

Discovery of an icy and nitrogen-rich extrasolar planetesimal

Snehalata Sahu, Boris T. Gänsicke, Jamie T. Williams +7

White dwarfs accreting planetary debris provide detailed insight into the bulk composition of rocky exo-planetesimals. However, only one Kuiper-Belt analogue has been identified in…

astro-ph.SR20252 cited

Precise Parameters for Two LISA Sources

Manuel Barrientos, Mukremin Kilic, Warren R. Brown +5

We present precise parameters for two compact double white dwarf binaries, SDSS J232230.20+050942.0 (J2322+0509) and SDSS J063449.92+380352.2 (J0634+3803), with orbital periods of…

astro-ph.SR20253 cited

A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon

Snehalata Sahu, Antoine Bédard, Boris T. Gänsicke +7

Atmospheric carbon has been detected in the optical spectra of six hydrogen-rich ultra-massive white dwarfs, revealing large carbon abundances (log C/H > 0.5) attributable to th…