MOST detects variability on τ Bootis A possibly induced by its planetary companion

2008/02/20 by Gordon A. H. Walker, G. A. H. Walker, Bryce Croll +16 · 6 citations
Physics and Astronomy · #Advanced Chemical Physics Studies #Astro and Planetary Science #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078952

7 pages, 7 figures; accepted for publication in A&A

arxiv created 2008/02/20 · openalex publication_date 2008/02/25 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30

Abstract

Context. There is considerable interest in the possible interaction between parent stars and giant planetary companions in 51 Peg-type systems.

Citations

• The MOST Asteroseismology Mission: Ultraprecise Photometry from Space
• Reduction of time-resolved space-based CCD photometry developed for MOST Fabry Imaging data

Cited by

• Magnetic field strengths of hot Jupiters from signals of star–planet interactions
• NONDETECTION OF POLARIZED, SCATTERED LIGHT FROM THE HD 189733b HOT JUPITER
• POSSIBLE CONSTRAINTS ON EXOPLANET MAGNETIC FIELD STRENGTHS FROM PLANET-STAR INTERACTION
• ROTATIONALLY MODULATEDg-MODES IN THE RAPIDLY ROTATING δ SCUTI STAR RASALHAGUE (α OPHIUCHI)
• Boötes [wikipedia]
• Planet [wikipedia]