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Limits to Tertiary Astrometric Companions in Binary Systems

Authors :
Muterspaugh, Matthew W.
Lane, Benjamin F.
Kulkarni, S. R.
Burke, B. F.
Colavita, M. M.
Shao, M.
Muterspaugh, Matthew W.
Lane, Benjamin F.
Kulkarni, S. R.
Burke, B. F.
Colavita, M. M.
Shao, M.
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