A new interferometric study of four exoplanet host stars:θ Cygni, 14 Andromedae,υAndromedae and 42 Draconis

2012/07/18 by R. Ligi, D. Mourard, A. M. Lagrange +20 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Exoplanet #Physics #Planet #RADIUS #Radial velocity #Stars #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201219467

published as 2012, A&A, 545, A5 · 10 pages + 2 pages appendix, 16 figures, accepted for publication in A&A

openalex publication_date 2012/07/18 · arxiv created 2012/08/19 · arxiv updated 2014/02/25 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Since the discovery of the first exoplanet in 1995 around a solar-type star, the interest in exoplanetary systems has kept increasing. Studying exoplanet host stars is of the utmost importance to establish the link between the presence of exoplanets around various types of stars and to understand the respective evolution of stars and exoplanets.

Citations

• Defining and cataloging exoplanets: the exoplanet.eu database
• Validation of the new Hipparcos reduction
• DIRECTLY DETERMINED LINEAR RADII AND EFFECTIVE TEMPERATURES OF EXOPLANET HOST STARS

Cited by

• STELLAR DIAMETERS AND TEMPERATURES. III. MAIN-SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS
• Andromeda (constellation) [wikipedia]