activity
19982024
most citedThe virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B

57 citations · 851 across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.SR2024

Spectral evolution of hot hybrid white dwarfs I. Spectral analysis

Semih Filiz, Klaus Werner, Thomas Rauch +1

Hydrogen-rich white dwarfs (WDs) comprise the majority of the WD population, but are only rarely found at the very hot end of the WD cooling sequence. A small subgroup that exhibit…

astro-ph.SR2024

Spectroscopic Survey of Faint Planetary-Nebula Nuclei. V. The EGB 6-Type Central Star of Abell 57

Howard E. Bond, Akshat S. Chaturvedi, Robin Ciardullo +3

During our spectroscopic survey of central stars of faint planetary nebulae (PNe), we found that the nucleus of Abell 57 exhibits strong nebular emission lines. Using synthetic nar…

astro-ph.SR2023

The photospheres of the hottest fastest stars in the Galaxy

Klaus Werner, Nicole Reindl, Thomas Rauch +2

We perform nonlocal thermodynamic equilibrium (NLTE) model atmosphere analyses of the three hottest hypervelocity stars (space velocities between 1500-2800 km s) k…

hep-ph2023

A New Model for Jet Energy Loss in Heavy Ion Collisions

Alexander Lind, Iurii Karpenko, Martin Rohrmoser +3

We present a new model for jet quenching from coherent radiation in a brick medium. The jet energy loss is simulated as a perturbative final-state vacuum parton shower followed by…

astro-ph.SR2018★ 32 cited

Spectral analysis of the extremely hot DA white dwarf PG0948+534

K. Werner, T. Rauch, N. Reindl

There is a striking paucity of hydrogen-rich (DA) white dwarfs (WDs) relative to their hydrogen-deficient (non-DA) counterparts at the very hot end of the WD cooling sequence. The…

astro-ph.SR2018★ 17 cited

Search for trans-iron elements in hot, helium-rich white dwarfs with the HST Cosmic Origins Spectrograph

D. Hoyer, T. Rauch., K. Werner +1

The metal abundances in the atmospheres of hot white dwarfs (WDs) entering the cooling sequence are determined by the preceding Asymptotic Giant Branch (AGB) evolutionary phase and…