Asteroseismology with the WIRE satellite

2006/09/26 by H. Bruntt, J. C. Suárez, J. C. Suarez +15
Physics and Astronomy · #Asteroseismology #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Geology #Photometer #Photometry (optics) #Physics #Remote sensing #Satellite #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065766

13 pages, 12 figures, 4 tables. Fig. 4 reduced in quality. Accepted by A&A

openalex publication_date 2006/09/26 · arxiv created 2006/10/18 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We have analysed ground-based multi-colour Strömgren photometry and single-filter photometry from the star tracker on the wire satellite of the δ Scuti star ϵ Cephei.

Citations

• Non-adiabatic theoretical observables inδScuti stars
• Theδ Scuti star XX Pyx is an ellipsoidal variable
• TheMOSTAsteroseismology Mission: Ultraprecise Photometry from Space
• Evidence for Granulation and Oscillations in Procyon from Photometry with theWIRESatellite
• Altair: The Brightest δ Scuti Star
• Detection of 75+ pulsation frequencies in theδScuti star FG Virginis