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Pulsating White Dwarfs

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arxiv 1706.07020 v1 pith:IQP6LM53 submitted 2017-06-21 astro-ph.SR

S. O. Kepler , Alejandra D. Romero This is my paper · ORCID
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keywords dwarfswhitepulsatingfactorfiveknownnumbervariable
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The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor of five and consequently the number of known pulsating white dwarfs also by a factor of five. It has also led to the discovery of new types of variable white dwarfs, as the variable hot DQs, and the pulsating Extremely Low Mass white dwarfs. With the Kepler Mission, it has been possible to discover new phenomena, the outbursts present in a few pulsating white dwarfs.

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  1. White dwarf-neutron star matter transition and the effect of light elements

    nucl-th 2026-08 conditional novelty 5.0 of 10

    A unified relativistic mean-field model connects white dwarfs to neutron stars and finds light-element seeds shift neutron star radii by roughly 0.2 km at 1.4 solar masses.

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