Precision astrometry of a sample of speckle binaries and multiples with the adaptive optics facilities at the Hale and Keck II telescopes

Monthly Notices of the Royal Astronomical Society

Volumn 400, Issue 1, 2009, Pages 406-421

  Helminiak K G ^a   Konacki, M ^a,b   Kulkarni, S R ^c   Eisner, J ^d  

^a NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^b ADAM MICKIEWICZ UNIVERSITY   (Poland)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

Author keywords

Astrometry; Binaries: Visual; Instrumentation: Adaptive optics; Planetary systems

Indexed keywords

ADAPTIVE OPTICS; INFRARED DEVICES; OBJECT DETECTION;

ASTROMETRIC PRECISION; ASTROMETRY; BINARIES:VISUAL; BINARY STAR; INSTRUMENTATION: ADAPTIVE OPTICS; MULTIPLE STARS; NEAR INFRARED; NEAR-INFRARED; PLANETARY MASS; PLANETARY SYSTEM;

STARS;

EID: 70449562405     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15495.x     Document Type: Article

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