A criterion for the occurrence of dynamical instability in the convective envelopes of red giants and AGE stars is presented. Using this criterion we find that the effect of turbulent pressure causes the dynamical instability in the regions very close to the surfaces of red giants and AGE stars, which affect the mass ejection outwards. This may be the mechanism powering the strong stellar winds of red giants and AGE stars with very low surface temperature and faint radiation pressure.
Jiang SY,Huang RQ. The effect of turbulent pressure on the red giants and AGB stars .2. On the mechanism powering the strong stellar winds[J]. ASTRONOMY & ASTROPHYSICS,1997,317(1):21-124.
APA
Jiang SY,&Huang RQ.(1997).The effect of turbulent pressure on the red giants and AGB stars .2. On the mechanism powering the strong stellar winds.ASTRONOMY & ASTROPHYSICS,317(1),21-124.
MLA
Jiang SY,et al."The effect of turbulent pressure on the red giants and AGB stars .2. On the mechanism powering the strong stellar winds".ASTRONOMY & ASTROPHYSICS 317.1(1997):21-124.
; Huang RQ(黄润乾)
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