HAL (France)
open access
Evolution of the near-core rotation frequency of 2497 intermediate-mass stars from their dominant gravito-inertial mode (Corrigendum)
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Delta Scuti stars in stellar systems: on the variability of HD 220392 and HD 220391#639575
- Multiple regular frequency spacings in $δ$ Scuti stars from automated analysis of TESS oscillation spectra#1116749
- A Universal Relation Between Primordial Density-Potential Cross-correlation Coefficient and Spin Factor Distribution#792789
- A Universal Relation Between Primordial Density-Potential Cross-correlation Coefficient and Spin Factor Distribution#788789
- Properties of rapidly rotating hot neutron stars within Brueckner theory#1156848
Record · ID 311966
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive