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HD 132753


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Analysis and solution of the light and radial velocity curves of the contact binary TY Bootis
Observations and analyses of the binary TY Bootis are presented. Radialvelocity data are used for the first time to establish the mass ratiowithout ambiguity, and an advanced version of the Wilson-Devinneysynthetic light curve program is used to analyze and solve the system. Areasonably robust set of parameters is obtained. TY Boo is found to be aW-type W UMa system with a mass ratio near two and a contact parameterof 0.12 + or - 0.903, indicating only shallow contact.

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Observation and Astrometry data

Constellation:Bootes
Right ascension:14h59m43.52s
Declination:+35°06'03.1"
Apparent magnitude:7.76
Distance:520.833 parsecs
Proper motion RA:-0.6
Proper motion Dec:-25.7
B-T magnitude:8.976
V-T magnitude:7.861

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 132753
TYCHO-2 2000TYC 2561-835-1
USNO-A2.0USNO-A2 1200-07438444
HIPHIP 73380

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