Radiative steady-state colliding stellar wind models: Are they correct?

Monthly Notices of the Royal Astronomical Society

Volumn 298, Issue 4, 1998, Pages 1021-1029

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

^a INSTITUTE FOR PROBLEMS IN MECHANICS   (Russian Federation)

^b Faculty of Physics Sofia University St Kliment Ohridski   (Bulgaria)

Author keywords

Binaries: general; Hydrodynamics; Instabilities; Shock waves

Indexed keywords

STABILITY; STARS;

BINARIES:GENERAL; BINARY SYSTEMS; MATHEMATICAL PROBLEMS; PROPERTY; SHOCK-WAVES; STABILITY PROPERTIES; STAGNATION POINTS; STEADY STATE; STELLAR WIND; WIND MODELLING;

SHOCK WAVES;

EID: 0000017955     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-8711.1998.01666.x     Document Type: Article

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