3 citations · 5 across the 5 of their papers we have counts for
5 papers
Forging neon-distilling white dwarfs in the stellar engulfments of helium white dwarfs
Nicholas Z. Rui, Jim Fuller
Once carbon--oxygen white dwarfs cool sufficiently, they crystallize from the inside out. If the white dwarf is rich enough in , these crystallized solids are b…
Seismology and diffusion of ultramassive white dwarf magnetic fields
Daniel Blatman, Nicholas Z. Rui, Sivan Ginzburg +1
Ultramassive white dwarfs (UMWDs; defined by masses ) are prime targets for seismology, because they pass through the ZZ Ceti instability strip at the s…
It's not just a phase: oblique pulsations in magnetic red giants and other stochastic oscillators
Nicholas Z. Rui, Jim Fuller, J. M. Joel Ong
Magnetic fields play a significant role in stellar evolution. In the last few years, asteroseismology has enabled the measurement of strong magnetic fields --$10^6\,\mathrm{G…
Magnetic dynamos powered by white dwarf superficial convection
Rom Yaakovyan, Sivan Ginzburg, Jim Fuller +1
When the effective temperature of a cooling white dwarf drops below the ionization limit, it develops a surface convection zone that may generate a magnetic field …
Supersensitive seismic magnetometry of white dwarfs
Nicholas Z. Rui, Jim Fuller, J. J. Hermes
The origin of magnetic fields in white dwarfs (WDs) remains mysterious. Magnetic WDs are traditionally associated with field strengths , set by the sensitivi…