Spectral analysis of Kepler SPB andβ Cephei candidate stars

2010/09/22 by H. Lehmann, A. Tkachenko, T. Semaan +9 · 1 citation
Engineering · Physics and Astronomy · #Asteroseismology #Astronomical Observations and Instrumentation #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Cepheid variable #Effective temperature #Instability strip #K-type main-sequence star #Metallicity #Photometry (optics) #Physics #Spectral line #Stars #Stellar, planetary, and galactic studies #T Tauri star #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201015769

10 pages, 10 figures, 10 tables

arxiv created 2010/09/22 · openalex publication_date 2010/12/03 · arxiv updated 2015/05/20 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. For asteroseismic modelling, analysis of the high-accuracy light curves delivered by the Kepler satellite mission needs support by ground-based, multi-colour and spectroscopic observations.

Citations

• Characteristics of 100+ Kepler Asteroseismic Targets from Ground-Based Observations
• Hydrogen and helium line formation in OB dwarfs and giants
• Effects of gravitational darkening on the determination of fundamentalparameters in fast-rotating B-type stars
• SELECTION, PRIORITIZATION, AND CHARACTERISTICS OF KEPLER TARGET STARS
• The Two Micron All Sky Survey (2MASS)
• A Grid of NLTE Line‐blanketed Model Atmospheres of Early B‐Type Stars
• The USNO-B Catalog

Cited by

• KIC 7177553: A QUADRUPLE SYSTEM OF TWO CLOSE BINARIES