Rotation of main-sequence stars at zero age and beyond

Details Rotation of main-sequence stars at zero age and beyond Rotation of main-sequence stars at zero age and beyond

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.5404b&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #54.04; Bulletin of the American Astronomical Society, Vol. 34, p.731

Astronomy and Astrophysics

Astronomy

Scientific paper

Rotation measurements of young main-sequence stars suggest a large range in rotation created by processes on the pre-main sequence. I will summarize and review these observations, as revealed by measurements in a series of open clusters, and draw attention to some deficiencies in the available dataset. Finally, I will also discuss the validity of some of the current beliefs in rotational evolution beyond the early stages.

Affiliated with

Also associated with

No associations

Rating

Rotation of main-sequence stars at zero age and beyond 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 Rotation of main-sequence stars at zero age and beyond, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotation of main-sequence stars at zero age and beyond will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1719083