Testing the Breakdown of the Asteroseismic Scaling Relations in Luminous Red Giants
Nearly all cool, evolved stars are solar-like oscillators, and fundamental stellar properties can be inferred from these oscillations with asteroseismology. Scaling relations are commonly used to relate global asteroseismic properties—the frequency of maximum power ${\nu }_{{\rm{\max }}}$ and the la...
Saved in:
Main Authors: | Amanda L. Ash, Marc H. Pinsonneault, Mathieu Vrard, Joel C. Zinn |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad9b18 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields
by: Marc H. Pinsonneault, et al.
Published: (2025-01-01) -
Signatures of Core-envelope Rotational Misalignment in the Mixed-mode Asteroseismology of Kepler-56
by: J. M. Joel Ong
Published: (2025-01-01) -
Tidally Distorted Stars Are Triaxial Pulsators
by: Jim Fuller, et al.
Published: (2025-01-01) -
A New Approach to Identifying Red Supergiant Stars in Metal-poor Galaxies: A Case Study of NGC 6822
by: Zhi-wen Li, et al.
Published: (2025-01-01) -
On the Age Calibration of Open Clusters Using Red Clump Stars
by: Abigail R. Chriss, et al.
Published: (2025-01-01)