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20242026
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astro-ph.SR2026

A systematic survey for hypervelocity runaways from thermonuclear supernovae

Kareem El-Badry, Klaus Werner, Ken J. Shen +16

The explosion of a white dwarf (WD) in a close binary can launch a surviving runaway star at velocities of . Such runaways provide a direct probe of…

astro-ph.SR2026

Spectroscopic survey of faint planetary-nebula nuclei. VII. Thirty new hydrogen-deficient central stars

Klaus Werner, Howard E. Bond, Gregory R. Zeimann

Our ongoing spectroscopic survey of faint planetary-nebula nuclei (PNNi) has revealed 30 new hydrogen-deficient central stars. The majority of them (21) belong to the PG1159 spectr…

astro-ph.SR2026

Spectral evolution of hot hybrid white dwarfs: II. Photometry

Semih Filiz, Nicole Reindl, David Jones +4

We present a photometric analysis of 19 DA and 13 DAO white dwarfs (WDs) with effective temperatures exceeding 60 kK, building on the spectral analysis reported in the first paper…

astro-ph.SR2025

How an overweight and rapidly rotating PG 1159 star in the Galactic halo challenges evolutionary models

Nina Mackensen, Nicole Reindl, Klaus Werner +2

PG 1159 stars are thought to be progenitors of the majority of H-deficient white dwarfs. Their unusual He-, C-, and O-dominated surface composition is typically believed to result…

astro-ph.SR2024

Three new hot hydrogen-deficient pre-white dwarfs

Klaus Werner, Nicole Reindl, Max Pritzkuleit +1

We have detected three new hydrogen-deficient (H < 0.001 mass fraction) pre-white dwarfs (WDs) with helium-dominated atmospheres. The first object is a relatively cool PG1159 star…

astro-ph.SR2024

An analysis of spectroscopic, seismological, astrometric, and photometric masses of pulsating white dwarf stars

Leila M. Calcaferro, Alejandro H. Córsico, Murat Uzundag +3

A central challenge in the field of stellar astrophysics lies in accurately determining the mass of isolated stars. However, for pulsating white dwarf (WD) stars, the task becomes…