The effect of turbulent pressure on the red giants and AGB stars. II. On the mechanism powering the strong stellar winds.

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Stars: Agb, Stars: Mass Loss, Instabilities

Scientific paper

A criterion for the occurrence of dynamical instability in the convective envelopes of red giants and AGB 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 AGB stars, which affect the mass ejection outwards. This may be the mechanism powering the strong stellar winds of red giants and AGB stars with very low surface temperature and faint radiation pressure.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The effect of turbulent pressure on the red giants and AGB stars. II. On the mechanism powering the strong stellar winds. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The effect of turbulent pressure on the red giants and AGB stars. II. On the mechanism powering the strong stellar winds., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effect of turbulent pressure on the red giants and AGB stars. II. On the mechanism powering the strong stellar winds. will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1780614

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.