Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475

Details Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475 Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..358..389f&link_type=abstract

Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Col

Physics

Scientific paper

Four probable Ap members of the open cluster NGC 6475, were investigated
through detailed spectrum synthesis. Cluster membership was confirmed
for all four stars, however chemical abundance analysis shows that only
three are truly Ap. Derived v sin i values and chemical abundances for
20 elements ranging form C to Eu are presented.

Affiliated with

Also associated with

No associations

Rating

Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475 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 and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotation and Chemical Abundances of Magnetic Ap/Bp Members in the Open Cluster NGC 6475 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1241062