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20152026
most citedFormation of Double Neutron Star Systems

698 citations · 1k across the 12 of their papers we have counts for

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astro-ph.SR2026

A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics

H. Dawson, M. Dorsch, S. Geier +30

We present a quantitative spectroscopic and kinematic analysis of a volume-complete sample of hot subluminous stars within 500 pc of the Sun, assembled using accurate parallax meas…

astro-ph.SR20251 cited

Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems

Larissa Antunes Amaral, Maja Vučković, Ingrid Pelisoli +3

In recent years, approximately 150 low-mass white dwarfs (WDs), typically with masses below 0.4 solar masses, have been discovered. Observational evidence indicates that most of th…

astro-ph.SR202214 cited

The impact of the uncertainties in the 12C(α,γ)16O reaction rate on the evolution of low- to intermediate-mass stars

Ben T. Pepper, A. G. Istrate, A. D. Romero +1

One of the largest uncertainties in stellar evolutionary computations is the accuracy of the considered reaction rates. The 12C(alpha,gamma)16O reaction is particularly important f…

astro-ph.SR202221 cited

Discovery of a highly magnetic He-sdO star from a double-degenerate binary merger

M. Dorsch, N. Reindl, I. Pelisoli +4

Helium-rich hot subdwarf stars of spectral type O (He-sdO) are considered prime candidates for stellar merger remnants. Such events should lead to the generation of strong magnetic…

astro-ph.SR2021

Pulsating hydrogen-deficient white dwarfs and pre-white dwarfs observed with TESS II. Discovery of two new GW Vir stars: TIC333432673 and TIC095332541

Murat Uzundag, Alejandro H. Córsico, S. O. Kepler +8

In this paper, we present the observations of two new GW Vir stars from the extended \textit{TESS} mission in both 120\,s short-cadence and 20\,s ultra-short-cadence mode of two pr…

astro-ph.SR2020

It has to be cool: on supergiant progenitors of binary black hole mergers from common-envelope evolution

J. Klencki, G. Nelemans, A. G. Istrate +1

Common-envelope (CE) evolution in massive binary systems is thought to be one of the most promising channels for the formation of compact binary mergers. In the case of merging bin…