Interior structura variations in the secondary components of two algol-type eclipsing binary systems: SW Cygni and RR Draconis

Astronomy and Astrophysics

Volumn 396, Issue 2, 2002, Pages 609-613

  Qian, S B ^a,b   Zhu, L Y ^a,b   Boonrucksar, S ^c  

^a Chinese Academy of Sciences   (China)

^b INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^c CHIANG MAI UNIVERSITY   (Thailand)

Author keywords

Stars: binaries: close; Stars: evolution; Stars: individual: RR Dra; Stars: individual: SW Cyg

Indexed keywords

HEAT CONVECTION; LIGHT EMISSION; MAGNETISM; MASS TRANSFER; SPECTROSCOPIC ANALYSIS;

ORBITAL PERIODS;

ASTROPHYSICS;

EID: 0036901867     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021387     Document Type: Article

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