2014/01/21 by Nancy Remage Evans, Evans, Nancy Remage
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR) #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1401.5440
To be published in the conference proceeding of " Setting a new standard in the analysis of binary stars", Leuven, 2013, (EAS) eds A. Tkachenko and K. Pavlovski
arxiv created 2014/01/21 · openalex publication_date 2014/01/21 · arxiv updated 2014/01/22 · openalex created_date 2022/09/11 · openalex updated_date 2026/07/28
Cepheids provide approaches to determining binary parameters which are often complementary to those for main sequence massive and intermediate mass stars. Specifically, we are using high resolution imaging, radial velocities, and X-ray studies to determine binary characteristics. Among the results are that they have both a high frequency of binary systems, and also a high proportion of triple systems.