arXiv (All)
open access
Ensemble pulsational characteristics of eclipsing binaries containing $β$ Cep stars observed by the TESS mission
Massive pulsators in eclipsing binaries provide precise, model-independent stellar parameters that, combined with asteroseismic constraints, provide powerful probes of interior properties and angular-momentum transport in massive stars. This study investigates the pulsational characteristics and the
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
- A search for dark companions around A-type stars via pulsation timing#1166514
- Investigating Potential Relationships Between Mass Transfer Indicators and $δ$ Scuti Pulsations in oEA Systems#985405
- VORTEX CREEP AND THE INTERNAL TEMPERATURE OF NEUTRON-STARS - TIMING NOISE IN PULSARS#212752
- Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies#314998
- Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? Implications for measurements of rotation and internal magnetic fields#415102
Record · ID 1156950
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