activity
19982022
most citedThe White Dwarf Luminosity Function from SDSS Imaging Data

196 citations · 1.9k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.SR2022★ 42 cited

The Merger Fraction of Ultramassive White Dwarfs

Mukremin Kilic, Adam G. Moss, Alekzander Kosakowski +6

We search for merger products among the 25 most massive white dwarfs in the Montreal White Dwarf Database 100 pc sample through follow-up spectroscopy and high-cadence photometry.…

astro-ph.SR2022★ 17 cited

The Rapid Rotation of the Strongly Magnetic Ultramassive White Dwarf EGGR 156

K. A. Williams, J. J. Hermes, Z. P. Vanderbosch

The distribution of white dwarf rotation periods provides a means for constraining angular momentum evolution during the late stages of stellar evolution, as well as insight into t…

astro-ph.SR2021★ 12 cited

The Initial-Final Mass Relation for Hydrogen-Deficient White Dwarfs

Joseph W. Barnett, Kurtis A. Williams, A. Bédard +1

The initial-final mass relation (IFMR) represents the total mass lost by a star during the entirety of its evolution from the zero age main sequence to the white dwarf cooling trac…

astro-ph.SR2021★ 15 cited

The White Dwarfs of the Old, Solar Metallicity Open Star Cluster Messier 67: Properties and Progenitors

Paul A. Canton, Kurtis A. Williams, Mukremin Kilic +1

The old, solar metallicity open cluster Messier 67 has long been considered a lynchpin in the study and understanding of the structure and evolution of solar-type stars. The same i…

astro-ph.SR2020★ 21 cited

The pulsating white dwarf G117-B15A: still the most stable optical clock known

S. O. Kepler, D. E. Winget, Zachary P. Vanderbosch +14

The pulsating hydrogen atmosphere white dwarf star G 117-B15A has been observed since 1974. Its main pulsation period at 215.19738823(63) s, observed in optical light curves, varie…

astro-ph.SR2020★ 1 cited

Ensemble Evolutionary Studies of White Dwarfs in Open Star Clusters

Kurtis A. Williams

White dwarfs (WDs) in open star clusters are a highly useful ensemble of stars. While numerous researchers use open cluster WDs to study the initial-final mass relation, numerous o…