2014/11/10 by G. Buldgen, Gaël Buldgen, Daniel Roy Reese +5
Physics and Astronomy · #Asteroseismology #Astro and Planetary Science #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Computer science #Context (archaeology) #Galaxy #Geology #Inversion (geology) #Physics #RADIUS #Seismology #Star formation #Stars #Stellar mass #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201424613
published as A&A 574, A42 (2015)
arxiv created 2014/11/10 · openalex publication_date 2014/11/26 · arxiv updated 2015/01/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Determining stellar characteristics such as the radius, mass or age is crucial when studying stellar evolution or exoplanetary systems, or when characterising stellar populations in the Galaxy. Asteroseismology is the golden path to accurately obtain these characteristics. In this context, a key question is how to make these methods less model-dependent.