Solar and Stellar Rotation

Details Solar and Stellar Rotation Solar and Stellar Rotation

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..370..169d&link_type=abstract

Solar and Stellar Physics Through Eclipses ASP Conference Series, Vol. 370, proceedings of the conference held 27-29 March, 2006

Physics

Scientific paper

The secular evolution of the stellar rotation through angular momentum loss, driven by the stellar wind, and the consequences of the angular momentum transfers between orbit and spinning components in binary star systems will be reviewed with the special emphasis on the Solar rotation. A large co-rotating distance (Alfvén radius) of the magnetically driven wind around single stars will be introduced to explain the large angular momentum loss from close binary star systems.

Affiliated with

Also associated with

No associations

Rating

Solar and Stellar Rotation 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 Solar and Stellar Rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar and Stellar Rotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-765494