Dissipative models of colliding stellar winds - I. Effects of thermal conduction in wide binary systems

Monthly Notices of the Royal Astronomical Society

Volumn 300, Issue 3, 1998, Pages 686-694

  Myasnikov, A V ^a   Zhekov, S A ^b  

^a INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

^b Bulgarian Academy of Sciences ^*  (Bulgaria)

Author keywords

Binaries: General; Hydrodynamics; Instabilities; Shock waves; Stars: Mass loss

Indexed keywords

GAS DYNAMICS; STARS; THERMAL CONDUCTIVITY; WIND;

BINARIES:GENERAL; BINARY SYSTEMS; DISSIPATIVE MODEL; HEATING ZONE; INTERACTION REGION; PRE-HEATING; SHOCK-WAVES; STARS: MASS-LOSS; STELLAR WIND; THERMAL CONDUCTION;

SHOCK WAVES;

EID: 0001525159     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-8711.1998.t01-1-01857.x     Document Type: Article

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