Well-resolved binary astrometry with the CHARA array

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 4838, Issue 2, 2002, Pages 1061-1067

  Bagnuolo Jr , W G ^a   Ten Brummelaar, T A ^b   McAlister, H A ^a   Turner, N H ^b   Sturmann, L ^b   Sturmann, J ^b   Ridgway, S T ^b  

^a GEORGIA STATE UNIVERSITY   (United States)

^b CHARA   (United States)

Author keywords

Binary stars; Infrared interferometry; Instrumentation; Optical interferometery; Reduction techniques

Indexed keywords

DATA REDUCTION; INFRARED RADIATION; INTERFEROMETERS; INTERFEROMETRY; MAXIMUM LIKELIHOOD ESTIMATION; SPECKLE;

BINARY ASTROMETRY;

ASTRONOMY;

EID: 0037877910     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.459078     Document Type: Conference Paper

References (6)

1. T.A. ten Brummelaar, "Technical update on the CHARA Array", SPIE (4006-68) (2000)
2. W.G. Bagnuolo and B. Mason, "Absolute Quadrant Determination from Speckle Observations of Binary Stars", AJ 103, 1399 (1992)
3. Barlow, D.J., Scarfe, C.D., Fekel, F.C., "Physical properites of the binary star 12 Persei", AJ 115, 325 (1998)
4. Pourbaix, D., "Resolved double-lined spectroscopic binaries: a neglected source of hypothesis-free parallaxes and stellar masses". Aamp;A Supp 145, 215 (2000)
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6. Martin, C., Mignard, F., Hartkopf, W.I., & McAlister, H.A. ''Mass Determination of Interferometric Binaries with Hipparhos III", Aamp;A Supp 133, 149 (1998)