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19922026
most citedThe Gaia mission

7.1k citations

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239 papers · 1 filter

astro-ph.SR2026★ 1 cited

Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries

Alberto Rebassa-Mansergas, Iset Tejero-Gómez, Roberto Raddi

The age-metallicity relation (AMR) is a fundamental observational constraint for understanding the chemical evolution of the Galaxy. As reliable cosmochronometers, white dwarfs in…

astro-ph.SR2026★ 2 cited

Extreme mass loss during common envelope evolution: the origin of the double low-mass white dwarf system J2102--4145

Leandro G. Althaus, Alejandro H. Corsico, Monica Zorotovic +3

Eclipsing close double white dwarf (WD) systems provide a unique opportunity to directly constrain hydrogen-envelope retention and test common-envelope (CE) evolution in low-mass s…

astro-ph.SR2026★ 1 cited

Constraints on White Dwarf Hydrogen Layer Masses Using Gravitational Redshifts

Stefan M. Arseneau, J. J. Hermes, Maria E. Camisassa +2

The hydrogen envelope is the outermost layer of a DA white dwarf; it makes up the entirety of the stellar photosphere, and yet its typical extent is difficult to model theoreticall…

astro-ph.SR2026

On the Importance of the Convective Urca Process in 3D Simulations of a Simmering White Dwarf

Ferran Poca-Amorós, Brendan Boyd, Dean M. Townsley +1

Type Ia supernovae are bright thermonuclear explosions that are important to numerous areas of astronomy. However, the origins of these events are poorly understood. One proposed s…

astro-ph.SR2026★ 2 cited

Gaia white dwarfs with infrared excess I. The 100 pc catalogue

R. Murillo-Ojeda, F. M. Jiménez-Esteban, A. Rebassa-Mansergas +1

The presence of infrared excess flux observed in white dwarfs (WDs) is related to the existence of debris disks or substellar companions. These systems provide important clues in t…

astro-ph.SR2026

Magnetohydrodynamic instabilities in stellar radiative regions. I. Linear study of shear-driven instabilities

V. Durepaire, L. Petitdemange, K. Belkacem +4

This paper is the first in a series investigating magnetohydrodynamic instabilities that may contribute to angular-momentum transport and magnetic-field evolution in stellar radiat…