q¹ Eridani: a solar-type star with a planet and a dust belt

2008/02/14 by R. Liseau, C. Risacher, A. Brandeker +9 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Astrophysics and Star Formation Studies #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079276

4 pages, 2 colour figures, Letter for Astronomy and Astrophysics, in press

openalex publication_date 2008/02/14 · arxiv created 2008/03/09 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

Context.Far-infrared excess emission from main-sequence stars is due to dust produced by orbiting minor bodies. In these disks, larger bodies, such as planets, may also be present and the understanding of their incidence and influence currently presents a challenge.

Citations

• The Extrasolar Planet ε Eridani b: Orbit and Mass
• NACO-SDI Direct Imaging Search for the Exoplanet ∊ Eri b
• Collisional processes and size distribution in spatially extended debris discs
• Catalog of Nearby Exoplanets
• The Geneva-Copenhagen survey of the Solar neighbourhood: Ages, metallicities, and kinematic properties of 14,000 F and G dwarfs

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• Disk Radii and Grain Sizes in Herschel-Resolved Debris Disks