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Rotation of White Dwarf Stars

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arxiv 1410.6934 v1 pith:7DCDHENE submitted 2014-10-25 astro-ph.SR

Steven D. Kawaler This is my paper · ORCID
classification astro-ph.SR
keywords starsdwarfevolutionrotationwhiteambiguitiesangularasteroseismology
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I discuss and consider the status of observational determinations of the rotation velocities of white dwarf stars via asteroseismology and spectroscopy. While these observations have important implications on our understanding of the angular momentum evolution of stars in their late stages of evolution, more direct methods are sorely needed to disentangle ambiguities.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 7 citations worldwide. Full citation record

  1. Zones of Tayler Instability in Stars

    astro-ph.SR 2024-11 conditional novelty 7.0 of 10

    New instability criteria for the Tayler instability with two types of stratification show a suppression layer around the hydrogen-burning shell in evolved low-mass stars and active instability at different wavenumbers...

  2. Sensitive Constraints on Coherent Radio Emission from Five Isolated White Dwarfs

    astro-ph.HE 2025-08 conditional novelty 6.0 of 10

    Sensitive searches of five isolated magnetic white dwarfs with FAST, GBT, and ATCA yield no radio emission, imposing the strongest constraints so far on isolated WD pulsars.

  3. Magnetic White Dwarfs in the SDSS 100 pc Sample: Further Evidence of Two Formation Channels

    astro-ph.SR 2025-07 conditional novelty 5.0 of 10

    A volume-limited sample of 163 magnetic white dwarfs separates into two populations, young/high-mass/strong-field and old/average-mass/weak-field, supporting two distinct formation channels.

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