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Gravitational Influence from Planets on the Measured Rates of Period Change of Pulsating White Dwarfs

The measured rates of period change, $\dot{P}$ , in the signals of pulsating white dwarf stars are often interpreted as direct detections of structural changes from secular cooling. Due to the intrinsic nature of this quantity, $\dot{P}$ analysis has been used to probe fundamental physics, such as c...

Ausführliche Beschreibung

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Bibliografische Detailangaben
Hauptverfasser: Ling Xuan Yao, Keaton J. Bell, Andrew Dublin
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/adfb66
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