Large-scale wind structure due to magnetic fields

Details Large-scale wind structure due to magnetic fields Large-scale wind structure due to magnetic fields

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cihw.conf..125u&link_type=abstract

Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Hamann, Wol

Computer Science

1

Scientific paper

Magnetic fields influence the dynamics of hot-star winds and create large scale structure. Based on numerical magnetohydrodynamic (MHD) simulations, we model the wind of θ¹ Ori C, and then use the SEI method to compute synthetic line profiles for a range of viewing angles as function of rotational phase. The resulting dynamic spectrum for a moderately strong line shows a distinct modulation, but with a phase that seems at odds with available observations.

Affiliated with

Also associated with

No associations

Rating

Large-scale wind structure due to magnetic fields 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 Large-scale wind structure due to magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Large-scale wind structure due to magnetic fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1340491