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Limits to Tertiary Astrometric Companions in Binary Systems
- Publication Year :
- 2006
-
Abstract
- The Palomar High-precision Astrometric Search for Exoplanet Systems (PHASES) has monitored 37 sub-arcsecond binary systems to determine whether their Keplerian orbits are perturbed by faint astrometric companions to either star. Software has been developed to evaluate the regions in a companion mass-period phase space in which the PHASES observations can exclude the possibility of face-on orbit perturbations. We present results for 8 systems for which astrometric companions with masses as small as those of giant planets can be excluded.<br />Comment: Accepted to ApJ, emulateapj 15 pages
Details
- Database :
- OAIster
- Publication Type :
- Electronic Resource
- Accession number :
- edsoai.ocn691217935
- Document Type :
- Electronic Resource
- Full Text :
- https://doi.org/10.1086.508743