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Amanda L. Ash

5 papers hereh-index 19 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
  • cs.CV1

identity via Semantic Scholar / OpenAlex

activity
20242026
most citedTesting the Breakdown of the Asteroseismic Scaling Relations in Luminous Red Giants

1 citations · 1 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

Modeling Rotation in the Old, Cold Domain: Implications on Gyrochronology and the Stellar Magnetic Wind

Amanda L. Ash, Yuxi, Lu +1

Gyrochronology ties stellar rotation periods to ages. It is well studied in the young, open cluster age domain, but there are few constraints on gyrochronology in the old field sta…

astro-ph.SR2025

Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion Relation

Yuxi Lu, Marc H. Pinsonneault, Yuan-Sen Ting +4

Determining stellar ages is challenging, as it depends on other stellar parameters in a non-linear way and often relies on stellar evolution models to infer the underlying relation…

astro-ph.SR2024★ 1 cited

Testing the Breakdown of the Asteroseismic Scaling Relations in Luminous Red Giants

Amanda L. Ash, Marc H. Pinsonneault, Mathieu Vrard +1

Nearly all cool, evolved stars are solar-like oscillators, and fundamental stellar properties can be inferred from these oscillations with asteroseismology. Scaling relations are c…

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