activity
19992017
most citedNew evolutionary models for massive ZZ Ceti stars: I. First results for their pulsational properties

109 citations · 748 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2017★ 27 cited

Evidence from K2 for rapid rotation in the descendant of an intermediate-mass star

J. J. Hermes, Steven D. Kawaler, A. D. Romero +9

Using patterns in the oscillation frequencies of a white dwarf observed by K2, we have measured the fastest rotation rate, 1.13(02) hr, of any isolated pulsating white dwarf known…

astro-ph.SR2016

Modeling the Spectra of Dense Hydrogen Plasmas: Beyond Occupation Probability

T. A. Gomez, M. H. Montgomery, T. Nagayama +2

Accurately measuring the masses of white dwarf stars is crucial in many astrophysical contexts (e.g., asteroseismology and cosmochronology). These masses are most commonly determin…

astro-ph.SR2016

Reaching Higher Densities for Laboratory White Dwarf Photospheres to Measure Spectroscopic Line Profiles

Ross E. Falcon, J. E. Bailey, T. A. Gomez +5

As part of our laboratory investigation of the theoretical line profiles used in white dwarf atmosphere models, we extend the electron-density () range measured by our e…

astro-ph.SR2016★ 5 cited

The First Six Outbursting Cool DA White Dwarf Pulsators

Keaton J. Bell, J. J. Hermes, M. H. Montgomery +4

Extensive observations from the Kepler spacecraft have recently revealed a new outburst phenomenon operating in cool pulsating DA (hydrogen atmosphere) white dwarfs (DAVs). With th…

astro-ph.SR2016★ 28 cited

Outbursts in two new cool pulsating DA white dwarfs

Keaton J. Bell, J. J. Hermes, M. H. Montgomery +9

The unprecedented extent of coverage provided by Kepler observations recently revealed outbursts in two hydrogen-atmosphere pulsating white dwarfs (DAVs) that cause hours-long incr…

astro-ph.SR2015★ 35 cited

A comparative analysis of the observed white dwarf cooling sequence from globular clusters

Fabíola Campos, P. Bergeron, A. D. Romero +8

We report our study of features at the observed red end of the white dwarf cooling sequences for three Galactic globular clusters: NGC\,6397, 47\,Tucanae and M\,4. We use deep colo…