Self-excited Pulsations and the Instability Strip of Long-period Variables: The Transition from Small-amplitude Red Giants to Semi-regular Variables

We use one-dimensional hydrodynamic calculations combined with synthetic stellar population models of the Magellanic Clouds to study the onset of self-excited pulsation in luminous red giants. By comparing the results with Optical Gravitational Lensing Experiment observations in the period–luminosit...

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Bibliographische Detailangaben
Hauptverfasser: Michele Trabucchi, Giada Pastorelli
Format: Artikel
Sprache:English
Veröffentlicht: IOP Publishing 2024-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online Zugang:https://doi.org/10.3847/1538-4357/ad9475