A possible relation between the period change and the mass ratio for W-type contact binaries

Monthly Notices of the Royal Astronomical Society

Volumn 328, Issue 2, 2001, Pages 635-644

  Qian, Shengbang ^a,b,c  

^a Chinese Academy of Sciences   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

Author keywords

Binaries: close; Stars: evolution; Stars: general

Indexed keywords

MASS TRANSFER;

ANGULAR MOMENTUM LOSS; BINARIES: CLOSE; CONTACT BINARIES; MASS RATIO; ORBITAL PERIODS; RELAXATION OSCILLATION; STAR: EVOLUTION; STARS: GENERAL; THERMAL RELAXATION; W-TYPES;

STARS;

EID: 0000641518     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04931.x     Document Type: Article

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