most citedObserving bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution

1 citations · 1 across the 1 of their papers we have counts for

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6 papers

astro-ph.SR20261 cited

Observing bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution

Murat Uzundag, Alejandro H. Corsico, Nicholas Jannsen +17

We present the scientific case for exploiting the capabilities of the PLATO mission to study bright pulsating white dwarfs across a wide spectral range, including hydrogen-deficien…

astro-ph.SR2026

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

Asteroseismology of the ZZ Ceti star WD 1310+583 using the Transiting Exoplanet Survey Satellite

Zs. Bognár, M. Uzundag, F. C. De Gerónimo +4

Aims. By analysing the light curves of the ZZ Ceti star WD 1310+583, we aim to determine its pulsational frequencies and to give constraints on the main stellar parameters using th…

astro-ph.IM2025

Asteroseismology of white dwarfs in the 2040s

Murat Uzundag, Ingrid Pelisoli, Stephane Charpinet +6

White dwarfs, the final evolutionary stage of the vast majority of stars, serve as critical tools for cosmochronology, studies of planetary system evolution, and laboratories for n…

astro-ph.SR2025

Asteroseismology of WD J004917.14-252556.81, the Most Massive Pulsating White Dwarf

O. Caliskan, M. Uzundag, M. Kilic +10

We present extensive follow-up time-series photometry of WD J00492525, the most massive pulsating white dwarf currently known with and $\log{\i…

astro-ph.SR2025

Discovery of the richest pulsating ultra-massive white dwarf

Francisco C. De Geronimo, Murat Uzundag, Alberto Rebassa-Mansergas +5

The discovery of pulsations in ultra-massive white dwarfs can help to probe their interiors and unveil their core composition and crystallized mass fraction through asteroseismic t…