Revising the ages of planet-hosting stars

2014/11/30 by A. Bonfanti, Andrea Bonfanti, S. Ortolani +5 · 3 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Space Science and Extraterrestrial Life #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201424951

published as A&A 575, A18 (2015) · 16 pages, 18 figures. Accepted by A&A

arxiv created 2014/12/05 · openalex publication_date 2014/12/05 · arxiv updated 2015/02/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04

Abstract

Aims. This article aims to measure the age of stars with planets (SWP) through stellar tracks and isochrones computed with the PAdova and TRieste Stellar Evolutionary Code (PARSEC).

Citations

• Y 2 Isochrones with an Improved Core Overshoot Treatment
• Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog
• Isochrone ages for field dwarfs: method and application to the age–metallicity relation
• Improved Age Estimation for Solar‐Type Dwarfs Using Activity‐Rotation Diagnostics
• The Ages of Stars
• The Exoplanet Orbit Database
• Basic physical parameters of a selected sample of evolved stars

Cited by

• Benchmark ages for theGaiabenchmark stars
• Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903
• Apus [wikipedia]